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Florida State University Libraries
2016
Characterizing the Onset and Demise of theIndian Summer MonsoonRyne Garrett Noska
Follow this and additional works at the FSU Digital Library. For more information, please contact [email protected]
FLORIDA STATE UNIVERSITY
COLLEGE OF ARTS AND SCIENCES
CHARACTERIZING THE ONSET AND DEMISE
OF THE INDIAN SUMMER MONSOON
By
RYNE G. NOSKA
A Thesis submitted to the Department of Earth, Ocean and Atmospheric Sciences
in partial fulfillment of the requirements for the degree of
Master of Science
2016
ii
Ryne G. Noska defended this thesis on March 24, 2016.
The members of the supervisory committee were:
Vasubandhu Misra
Professor Directing Thesis
Robert Hart
Committee Member
Mark Bourassa
Committee Member
The Graduate school has verified and approved the above-named committee members, and
certifies that the thesis has been approved in accordance with university requirements.
iii
I dedicate this work to
Jesus
The Rock of Ages
Upon whom I stood
In the midst of the deluge
During these formative years of my life:
You never fail me!
“From the end of the earth
I call to You when my heart is faint;
Lead me to the rock that is higher than I.”
~Psalm 61:2
iv
ACKNOWLEDGMENTS
I am grateful first and foremost for my Lord Jesus Christ, who has been a firm
foundation throughout my stay at Florida State University. I would find no purpose in my
research or in anything else without Him, for in Him I live and move and have my being. My
family, and especially my wife Jenna, were invaluable during my graduate years. They
reminded me of the world outside of meteorology and that I should, indeed must, be engaged
in it. What a joy it is to be reminded of what matters most in life through their affection and
support!
I thank Dr. Vasubandhu Misra for his willingness to guide me as I encountered
complex challenges and to offer suggestions that further improved my research. I do not doubt
that I completed so much research in such a short period of time because of your motivating
encouragement. Drs. Bob Hart and Mark Bourassa have also offered many suggestions and
corrections that made the outcome of my research much greater than it began; thank you. I
further acknowledge the immense assistance Drs. Amit Bhardwaj and Akhilesh Mishra
offered through many useful discussions and programming support; I consider you both as
friends.
I gratefully acknowledge the financial support given by NOAA (NA12OAR43310078)
and the Earth System Science Organization, Ministry of Earth Sciences, Government of India
(Grant number MM/SERP/FSU/2014/SSC-02/002) to conduct this research under Monsoon
Mission. Finally, I thank the Indian Meteorological Department for the availability of the
daily rain analysis over India.
v
TABLE OF CONTENTS
List of Tables ............................................................................................................................ vi List of Figures ......................................................................................................................... vii Abstract ..................................................................................................................................... x 1. INTRODUCTION ................................................................................................................ 1 2. DATA ................................................................................................................................... 5 3. METHODOLOGY ................................................................................................................ 9
3.1. Defining the All-India Rainfall Onset and Demise Index............................................ 9 3.2. Insensitivity to False Onsets ...................................................................................... 11 3.3. Seasonal Evolution ..................................................................................................... 13 3.4. Interannual Variability .............................................................................................. 16
4. RESULTS AND DISCUSSION ......................................................................................... 19
4.1. Insensitivity to Arbitrary Domain Changes, Time Period Changes, and False Onsets ......................................................................................................................... 19
4.2. Seasonal Evolution ..................................................................................................... 20 4.2.1 The Land-Ocean Temperature Contrast ........................................................ 23 4.2.2 Large-Scale Atmospheric Circulation Reversal .............................................. 24 4.2.3 Large-Scale Oceanic Circulation Reversal ..................................................... 25 4.2.4 Moisture Convergence and Subsequent Precipitation ................................... 28
4.3. Interannual Variability .............................................................................................. 30 4.3.1 Features of the Indian Summer Monsoon ...................................................... 30 4.3.2 Temperature .................................................................................................... 32 4.3.3 Wind ................................................................................................................ 33 4.3.4 Oceanic Phenomena ........................................................................................ 34 4.3.5 Moisture........................................................................................................... 35
5. CONCLUSION .................................................................................................................. 38 APPENDICES ......................................................................................................................... 41 A. Tables ................................................................................................................................. 41 B. Figures ............................................................................................................................... 49 References ................................................................................................................................ 90 Biographical Sketch................................................................................................................. 96
vi
LIST OF TABLES
1 Large-scale atmospheric and oceanic changes associated with onset from previous literature. .......................................................................................................................... 41
2 Onset indices from previous literature. ........................................................................... 43
3 Datasets implemented in this paper and their metadata. ............................................ 45
4 False onset years and their three pertinent dates: false onset, “actual” onset, and AIRO. ................................................................................................................................ 45
5 Direct and derived large-scale atmospheric and oceanic variables analyzed in this
study. ................................................................................................................................. 46
6 Correlations between ISM features. Bolded values are significant at the 95% confidence interval. ............................................................................................................................. 46
7 Annual total seasonal AIR, AIRO, AIRD, and season length. ......................................... 47
vii
LIST OF FIGURES 1 Important locations referred to during this study. .......................................................... 49 2 The domains and rain gauge distributions used in APHRODITE V1101 for monsoon
Asia (MA), the MIddle East (ME), and northern Eurasia [i.e., Russia (RU)], and in V1005 for Japan (JP). ........................................................................................................ 49
3 Seasonal cycle of rainfall for the year 2000. ................................................................. 50 4 The seasonal cycle of rainfall during the Maharashtra Drought of 1972. ...................... 50 5 OLR in the middle of May for the four cases of multiple monsoon onset. ....................... 51 6 AIR-based a) onset date, b) demise date, and c) season length from 1902 to 2005. ........ 52 7 Distribution of onset dates (top), demise dates (middle), and season length (bottom). .. 53
8 Parameters characterizing a Gaussian or normal distribution. ....................................... 54 9 Brown shaded area represents the AIR region. ................................................................ 55
10 Comparison of onset (top) and demise (bottom) dates for two spatially-averaged rainfall
domains: AIR and APHRO. .............................................................................................. 56 11 Seasonal evolution of 11 false onset years recorded by previous studies. ....................... 57
12 Ekman transport throughout the mixed layer (roughly 100m) of the ocean, where the
competing Coriolis force and turbulent drag slow and turn the direction of the current to the right at deeper depths. ............................................................................................... 58
13 Simplified regulation of the seasonal cycle of the Indian Ocean in the boreal a) summer
and b) winter, where black arrows indicate the direction of near-surface winds and gray arrows indicated the direction of Ekman transport and the resulting heat flux. ........... 58
14 Seasonal evolution of the daily composite (averaged over 104 years from 1902-2005) of
300hPa temperature centered on the AIRO (time = 0) at intervals of five days. ............ 59
15 Same as Fig. 14, but centered on the AIRD. .................................................................... 60
16 The climatological daily zonal progression of the meridional temperature gradient between 5°N and 25°N at 300hPa as a function of lead/lag time with respect to the a) AIRO and b) AIRD from 40°E to 120°E. ........................................................................... 61
17 Same as Fig. 14, but for 850hPa to 200hPa vertical wind shear. .................................... 62
18 Same as Fig. 14, but for 850hPa to 200hPa vertical wind shear centered on the AIRD. ................................................................................................................................ 63
viii
19 Same as Fig. 14, but for kinetic energy of 850hPa winds. ............................................... 64 20 Same as Fig. 14, but for kinetic energy of 850hPa winds centered on the AIRD. ........... 65
21 The climatological daily meridional progression of zonally-averaged meridional ocean
heat transport computed to a depth of 105m (~mixed layer depth of the tropical Indian Ocean) as a function of lead/lag time with respect to the a) AIRO and b) AIRD from 25°S to 25°N. ............................................................................................................................. 66
22 Schematic of the horizontal velocity structure of the n=1 Rossby mode with southward
Ekman flow added to regions outside of the equatorial wave guide and cool colored pathways and streamlines indicating southward heat transport. .................................. 66
23 Same as Fig. 14, but for vertically integrated moisture flux convergence. ..................... 67
24 Same as Fig. 14, but for vertically integrated moisture flux convergence centered on the
AIRD. ................................................................................................................................ 68
25 Same as Fig. 14, but for precipitable water. .................................................................... 69
26 Same as Fig. 14, but for precipitable water centered on the AIRD. ................................ 70
27 Same as Fig. 14, but for rainfall. ...................................................................................... 71
28 Same as Fig. 14, but for rainfall centered on the AIRD. ................................................. 72
29 Correlation of a) AIRO and b) AIRD date anomalies with total seasonal rainfall anomalies. ......................................................................................................................... 73
30 Same as Fig. 29, but with 300hPa meridional temperature gradient from 5°N to 25°N at
various lead/lag times with respect to the a) AIRO and b) AIRD date. .......................... 73
31 Correlation of AIRO date anomalies with 300hPa temperature anomalies at various lead/lag times. ................................................................................................................... 74
32 Same as Fig. 31, but with AIRD date anomalies. ............................................................ 75
33 Same as Fig. 31, but with 850hPa to 200hPa vertical wind shear anomalies. ............... 76
34 Same as Fig. 31, but with 850hPa to 200hPa vertical wind shear anomalies and AIRD
date anomalies. ................................................................................................................. 77
35 Same as Fig. 31, but with kinetic energy anomalies of 850hPa wind. ............................ 78
36 Same as Fig. 31, but with kinetic energy anomalies of 850hPa wind and AIRD date anomalies. ......................................................................................................................... 79
37 Same as Fig. 29, but with meridional ocean heat transport from 25°S to 25°N at various
lead/lag times with respect to the a) AIRO and b) AIRD date. ........................................ 80
ix
38 Correlation of AIRO date anomalies with global December-February averaged sea surface temperature anomalies. ....................................................................................... 80
39 Correlation of monthly Niño3.4 sea surface temperature (SST) anomalies with AIRO
date anomalies (red circles), AIRD date anomalies (black squares), total seasonal AIR anomalies (blue circles), and June-September (JJAS) AIR anomalies (green
diamonds). ......................................................................................................................... 81
40 A comparison of the total seasonal AIR (blue) and the June-September (JJAS) All-India Monsoon Rainfall (AIMR; orange). ................................................................................... 82
41 Same as Fig. 31, but with vertically integrated moisture flux convergence anomalies. ......................................................................................................................... 83
42 Same as Fig. 31, but with vertically integrated moisture flux convergence anomalies
and AIRD anomalies. ........................................................................................................ 84
43 Same as Fig. 31, but with precipitable water anomalies. ................................................ 85
44 Same as Fig. 31, but with precipitable water anomalies and AIRD anomalies. ............. 86
45 Same as Fig. 29, but with AIR anomalies at various lead/lag times with respect to the a) AIRO and b) AIRD date. ................................................................................................... 87
46 Same as Fig. 31, but with rainfall anomalies. ................................................................. 88
47 Same as Fig. 31, but with rainfall anomalies and AIRD date anomalies. ...................... 89
x
ABSTRACT
An objective index of the onset and demise of the Indian summer monsoon (ISM) is
introduced. This index has the advantage of simplicity by using only one readily available
variable, All-India rainfall (AIR), which has been reliably observed for more than a century.
The proposed All-India rainfall onset and demise (AIROD) is shown to be insensitive to all
recorded false onsets. By definition, the seasonal ISM rainfall anomalies become a function
of the variations of onset and demise dates, with early onset and late demise resulting in
greater season length and total seasonal rainfall. Seasonal rainfall itself is a strong predictor
of the following ENSO phase and provides a more accurate depiction of the ISM than does
the commonly-used June-September (JJAS) All-India monsoon rainfall (AIMR) index.
This new index provides an accurate and comprehensive representation of the
seasonal evolution of the ISM by capturing dramatic changes in large-scale dynamic (i.e.
wind- and current-based) and thermodynamic (temperature- and moisture-based) variables,
which is found to make the onset an especially important feature to monitor to understand
the evolution of the ensuing monsoon season. In particular, the zonal (meridional)
progression of 300hPa meridional temperature gradient (meridional ocean heat transport)
reversal may be monitored about twenty days before onset to help determine the timing of
its arrival.
Interannual variability of ISM features and their associated large-scale phenomena
are also analyzed. An early (late) onset corresponds to an increase (decrease) in anomalies of
kinetic energy of 850hPa wind over the Arabian Sea and central Indian rainfall up to fifteen
and ten days before onset, respectively. Conversely, an early (late) demise corresponds to a
decrease (increase) in the aforementioned anomalies up to ten days after demise.
xi
Additionally, the preceding December-February ENSO phase is associated with the onset of
the ISM, as an early (late) onset is preceded by La Niña (El Niño).
1
CHAPTER 1
INTRODUCTION The Indian summer monsoon (ISM), which is derived from the Arabic word translated
“season”, is defined as the reversal of the large-scale wind pattern to southwesterlies off the
Somali Coast. A sudden increase in rainfall occurs as a visible manifestation of this shift in
wind direction and impacts many aspects of Indian society. The ISM, which climatologically
occurs from June to September, affects over 1.25 billion people in India, providing 70-90% of
the nation’s annual mean rainfall (Kumar et al., 2013). Agriculture, which accounts for over
20% of India’s gross domestic product and employs over half of its workforce, is particularly
impacted as over 60% of agricultural production is rain-fed by the monsoon (Kumar et al.,
2004). Therefore a comprehensive understanding and consequent accurate prediction of
monsoon characteristics are essential.
The onset and demise of the ISM in particular are of such importance that the Indian
Meteorological Department (IMD) has determined them for more than 100 years
(Ananthakrishnan and Soman, 1988; Pai and Rajeevan, 2009). These transitions are
associated with significant changes in large-scale atmospheric and oceanic phenomena, and
their potentially unanticipated variability oftentimes leads to economic, agricultural,
governmental, and societal stress (Gadgil and Kumar, 2006). Some of the most drastic
changes occur with temperature, wind, moisture, and oceanic variables (Table 1). Many onset
and demise indices have been suggested in an attempt to accurately portray these essential
features of the ISM (Table 2). While onset and demise dates are not unique in that they may
be determined using a number of indices and variables, any suggested index should capture
the aforementioned drastic, large-scale atmospheric and oceanic changes.
2
There are a number of limitations for previously suggested onset and demise indices.
Without objective thresholds, an index cannot provide an exact date of onset and is subject
to forecaster bias (Rao, 1976). Second, many indices consider a single variable without
providing an atmospheric and oceanic context, which may result in a narrow scope of
application (Ananthakrishnan et al., 1968; Ramage, 1971; Ananthakrishnan and Soman,
1988; Fasullo and Webster, 2003; Janowiak and Xie, 2003; Zeng and Lu, 2004; Taniguchi and
Koike, 2006; Xavier et al., 2007; Wang et al., 2009; Goswami and Gouda, 2010; Moron and
Robertson, 2014; Misra and DiNapoli, 2014). Fasullo and Webster (2003) argues that onset
and demise dates based on rainfall alone are susceptible to both poor measurements and
modeling, which vertically integrated moisture transport ameliorates. On the other hand, the
hydrological index as suggested in Fasullo and Webster (2003), among many others,
encounters difficulty in capturing the synoptic variability and spatial complexity of monsoon
transitions (Ramage, 1971; Zeng and Lu, 2004; Prasad and Hayashi, 2005; Taniguchi and
Koike, 2006; Xavier et al., 2007; Wang et al., 2009).
Another critical limitation is susceptibility to false onsets (Ananthakrishnan et al.,
1968; Ramage, 1971; Rao, 1976; Ananthakrishnan and Soman, 1988; Wang et al, 2009;
Goswami and Gouda, 2010; Misra and DiNapoli, 2014). A false onset is a brief increase in
rainfall that precedes onset and is followed by a lengthened period of dryness (Joseph et al.,
1994; Flatau et al., 2001, 2003; Moron and Robertson, 2014). False onsets are also referred
to in scientific studies as double onsets, bogus onsets, and pre-monsoon rain peaks (PMRP)
(Joseph and Pillai, 1988; Flatau et al., 2001; Fasullo and Webster, 2003; Pai and Rajeevan,
2009). Such occurrences are a result of synoptic disturbances on small time scales; thus, any
index which does not cover a large enough region and time period is likely susceptible.
Similarly, many indices account only for Kerala, a small region on the southwestern tip of
the Indian subcontinent, and therefore are not necessarily indicative of onset for the region
3
as a whole (Ananthakrishnan et al., 1968; Rao, 1976; Ananthakrishnan and Soman, 1988;
Joseph et al., 2006; Pai and Rajeevan, 2009; Goswami and Gouda, 2010).
As Fasullo and Webster (2003) mention, some indices are also based upon poor
measurements or time steps much longer than the daily time step for which onset and
withdrawal occur (Rao, 1976; Janowiak and Xie, 2003; Zeng and Lu, 2004). While these
limitations are sufficient for coarse global studies, practical applications require better
resolution and data density. Contemporary datasets and models allow this limitation to be
overcome (Rajeevan et al., 2008; Saha et al., 2010; Yatagain et al., 2012). Finally, many
indices are not intended for forecasting purposes but rather for modeling and research
applications, usually as a result of a variable’s required persistence (Ramage, 1971;
Ananthakrishnana and Soman, 1988; Janowiak and Xie, 2003; Zeng and Lu, 2004; Taniguchi
and Koike, 2006; Wang et al., 2009; Goswami and Gouda, 2010; Moron and Robertson, 2014;
Misra and DiNapoli, 2014). While the index explored in this study provides no objective
solution to this limitation, it shall be shown that subjective monitoring may be possible.
A new index for onset and demise based on IMD daily rainfall over the entire Indian
subcontinent is introduced for the following reasons: 1) rainfall exerts a practical influence
on all sectors of Indian society; 2) those outside the scientific community have greater
comprehension and experience of a precipitation-based index; 3) rainfall is one of few directly
and reliably observed daily variables available since the early twentieth century over India,
4) the selected region is large enough and the rainfall threshold robust enough to avoid
synoptic-triggered false onsets; and 5) the IMD gridded rainfall dataset implemented has
excellent spatiotemporal resolution. A daily precipitation-based onset date is also easily
comparable to the IMD onset definition. However, the larger domain for all-India rainfall
(AIR) should result in later onset dates than IMD rainfall, which only considers preliminary
rainfall in Kerala, and should thus be more representative of India’s collective onset and
4
demise dates and more resistant to false onsets. All large-scale atmospheric and oceanic
changes are then characterized in this new index’s context to provide a comprehensive view
of monsoon transitions, a view which is lacking in most other previous studies. In this way,
numerous variables instead of rainfall alone are used to portray its far-reaching implications
and its accurate representation of large-scale atmospheric and oceanic changes.
Furthermore, the index suggested is flexible in that it may be applied to any strongly seasonal
variable of interest. Fasullo and Webster (2003) provides the following criteria that every
successful onset and demise index must meet:
association with transition of large-scale monsoon circulation processes;
insensitivity to fluctuations within the monsoon season and to false onsets caused by
individual synoptic disturbances; and
foundation upon well-observed, long-duration fields that experience sudden, extreme
variability during monsoon transitions.
The onset and demise index presented in this study meets each condition in a clear and
applicable fashion.
This study objectively determines the onset and demise of the Indian summer
monsoon in a manner that avoids false onsets, allows holistic characterization of and real-
time monitoring of seasonal evolution, and accurately captures interannual variability.
Chapter 2 reviews the datasets used in this research. The methodology implemented to
determine and characterize onset and demise dates is elucidated in chapter 3. Results
concerning the index’s insensitivity to false onsets, the seasonal evolution of the ISM, and
the variability of features of the ISM are discussed in chapter 4. Conclusions are included in
the final chapter.
5
CHAPTER 2
DATA
Different datasets are used for atmospheric and oceanic variables (Table 3). Gridded
AIR is obtained from the Indian Meteorological Department (IMD) National Climate Centre
(NCC) 0.25° gridded rainfall dataset (Pai et al., 2014a,b), which was directly provided by a
known contact at the NCC for the years 1902 to 2005. The data is interpolated to a 0.25° grid
spacing using over 2,500 quality-controlled stations (Pai et al., 2014a,b). Recall that this
rainfall is one of the only directly observable daily variables during the full 104 years of this
study over India. In order to ensure the resistance of the rainfall-based onset and demise
dates to changes in domain, the Research Institute for Humanity and Nature (RIHN) and
Meteorological Research Institute of Japan Meteorological Agency’s (MRI/JMA) Asian
Precipitation – Highly Resolved Observational Data Integration Towards Evaluation of
Water Resources (APHRODITE) version 1101 station data was compared to IMD AIR. The
station data was interpolated to 0.25 grid spacing from 1951-2005 and included both India
and Bangladesh in its domain (Yatagai et al., 2012). This data was supplied and downloaded
from the Center for Ocean and Atmospheric Prediction Studies (COAPS) at Florida State
University (FSU). Caution should be taken with gridded data as the density of stations are
not homogenous throughout the region of study. Note that there are far fewer stations in
eastern India and southeastern Bangladesh as can be seen in Fig. 2.
All other atmospheric variables were downloaded by batch from the European Centre
for Medium-Range Weather Forecasts’ (ECMWF) Atmospheric Reanalysis of the 20th
Century (ERA-20C; Poli et al., 2013), ECMWF’s first extended climate reanalysis (Dee et al.,
2014), using the python library “ecmwfapi”. Only surface observations are assimilated using
an Ensemble of Data Assimilations (EDA) of 10 members which are forced by a HadISST
6
2.1.0.0 ensemble of sea-surface temperature and sea-ice conditions. Each member employs a
24-hour four-dimensional variational (4D-Var) analysis scheme. Assimilated surface
observations are provided by the International Surface Pressure Databank (ISPD) 3.2.6
(atmospheric surface pressure) and the International Comprehensive Ocean-Atmosphere
Data Set (ICOADS) 2.5.1 (atmospheric surface pressure, atmospheric and ocean
temperatures, and atmospheric near-surface winds all only above oceans). The pressure
observations are bias-corrected using a variational bias correction within the assimilation,
and the wind observations above oceans are assimilated as they are verified to improve the
quality of the atmospheric circulation representation, particularly in the tropics (Poli et al.,
2013). This dataset is interpolated from approximately 125km resolution (using a spectral
triangular truncation T159) and 3-hour time step to a 0.25 grid spacing and daily time step
from 1902 to 2005 to match the observational rainfall’s spatiotemporal gridding. The domain
for precipitable water, vertically integrated moisture flux divergence, and the zonal and
meridional components of wind velocity is 50-110E and 0-40N. 300hPa temperature’s
longitudinal extent is broadened from 40-120E so that all pertinent information noted by
Yanai et al. (1992) is accounted for.
A few cautionary statements must be made concerning this relatively new
atmospheric reanalysis. First, data in the upper tropospheric/lower stratospheric 100-200hPa
levels are to be viewed with caution as they are highly model-dependent (Poli et al., 2013).
All validation conducted in this study, with the exception of 850-200hPa vertical wind shear,
are in the lower troposphere (well below these cautionary levels). Second, long-term climate
trends are not completely captured by the reanalysis, which produces increments away from
the surface due to insufficient attention during system development to diagnose the quality
of low-frequency climate information in advance (Poli et al., 2015). Poli et al. (2013) does
7
indicate, however, that representation of daily meteorological events, including extremes, is
of reasonable quality. ERA-20C seems to be an excellent reanalysis for this study because
the primary focus of this research is on a daily time scale and large variations in variables
rather than with exact quantities are desired. Quantitative errors are not as crucial as errors
in pattern representation, and as previously stated the reanalysis accurately portrays daily
events. It is also the only reanalysis available at T159 (125km) resolution for over a century
and is conducted with a relatively modern version of the ECMWF model which incorporates
4D-variational analysis. Finally, ERA-20C is a pilot reanalysis, and is not intended to
produce a final ‘best-product’ state-of-the-art climate dataset. Rather, its primary purpose is
the study of the feasibility of reanalyzing the century using new data assimilation methods
to tackle the problem of observing system changes (Poli et al., 2013). As indicated above,
however, the atmospheric reanalysis performs very well on the daily timescale and is thus
effective for this research.
Meridional ocean current and potential temperature are extracted from the National
Centers for Environmental Prediction’s (NCEP) Climate Forecast System Reanalysis (CFSR;
Saha et al., 2010), the first global reanalysis based on a coupled model of the atmosphere-
ocean-land surface-sea ice system. This data, as with APHRODITE, is available from COAPS
at FSU. Its assimilation scheme is considered weakly coupled in that it uses the coupled
model only for generating background estimates for each analysis cycle while the analysis
itself is uncoupled. As a result, information from observations in any one component can only
affect other components indirectly by propagating information to the next analysis cycle (Dee
et al., 2014). The resolution is 0.25 at the equator, but resolution decreases to 0.5 beyond
the tropics (Saha et al., 2010). Therefore, all data ingested in this study was interpolated to
a uniform 0.5 grid spacing for consistency. Potential temperature and meridional current
8
velocity were calculated for a domain of 40-100E and 25S-25N. Eleven of the available
forty depth levels were used, down to a depth of 105m., and the variables were computed
daily from 1979 to 2005. The Met Office Hadley Centre’s sea ice and sea surface temperature
(SST) data set version 1 (HadISST1; Rayner et al., 2003; Reynolds et al., 2007) is available
from COAPS at FSU and provides 1 square grids of monthly-averaged, global SSTs from
1871 to the present, but only years since 1902 are used in this study for comparison with the
primary dataset, IMD AIR. Finally, the National Center for Atmospheric Research (NCAR)
Climate and Global Dynamics (CGD) Climate Analysis Section (CAS) supplies a record of
Niño 3.4 monthly SSTs (N3.4) (Trenberth and Stepaniak, 2000). The domain over which the
Niño 3.4 SSTs are averaged extends from 170W to 120W and from 5S to 5N, and the years
from 1902 to 2005 are extracted from the record as a text file by copying values from
http://www.cgd.ucar.edu/cas/catalog/climind/TNI_N34/.
All analysis was completed using the Formula Translating System (FORTRAN) 95
programming language and visualized with the Grid Analysis and Display System (GrADS)
2.0, the Matrix Laboratory (MATLAB), and Microsoft Excel.
9
CHAPTER 3
METHODOLOGY
3.1 Defining the All-India Rainfall Onset and Demise Index
The onset and demise of the Indian summer monsoon (ISM) are herein determined
using observed daily rainfall. Following Liebmann et al. (2007) and Misra and DiNapoli
(2014), a cumulative daily anomaly of rainfall � �� is computed as � �� = ∑ [ − ̅]��= , (1)
where is the daily rainfall on day and ̅ is the annual mean of rainfall. Onset (demise)
is determined as the first day exceeding (falling below) the annual mean, or the day after the
first minimum (maximum) of anomalous accumulation. Unfortunately, while this index
works well for slowly varying variables such as sea surface temperature, it does not eliminate
false onsets for noisy, or quickly changing, variables. For example, rainfall can suddenly yet
briefly increase as a result of a synoptic-scale system, resulting in the first day of excessive
rainfall relative to the annual mean and thus producing a false onset. Furthermore,
interannual comparison is not possible as onset and demise are determined by the annual
mean threshold which changes each year. Finally, such an annual mean requires the data
from the beginning to the end of a given year, thus prohibiting any attempt at real-time
monitoring of the ISM.
Two steps are taken to alleviate these limitations. First, the annual mean rainfall in
equation (1) is replaced with the climatological annual mean rainfall; that is, the annual
mean rainfall is computed for each year, and then an individual climatological value is
calculated by averaging the annual mean rainfall values. This change allows for interannual
comparison, and also permits real-time monitoring since the climatological annual mean
10
rainfall value is available in advance of the ISM. Equation (1) may thus be adapted to the
following general format:
′ = ∑ [ � − ̿]�= . (2)
′ is the cumulative daily anomaly of AIR through day n of year m, � is the daily AIR
for day � of year , and ̿ is the annual mean climatology of AIR. These three terms are
plotted in Fig. 3 for the year 2000 as an illustrative example of the seasonal cycle of AIR.
Note that equation (2) may be expressed for any variable that exhibits strong seasonality,
but is expressed for AIR in the current study. A second step is taken to render the index
insusceptible to false onsets. Rather than the AIR-based onset (demise) date being
determined as the day after the first minimum (maximum) of the cumulative daily anomaly,
it is defined as the day after the absolute minimum (maximum) of the cumulative daily
anomaly. In this manner, false onsets are avoided because exceedance of climatological
annual mean rainfall for a short period of time followed by a deficit in rainfall will not result
in the lowest minimum cumulative daily anomaly of AIR.
A couple of additional stipulations must be imposed upon the index above to prevent
incorrect detection of onset and demise dates, especially during anomalously dry years. In
such years it is potentially possible to come up with a zero length of the monsoon season as
the onset (demise) date could reside on the last (first) day of the year due to the cumulative
daily anomaly of AIR for that year remaining below (above) the true onset (demise) minimum
(maximum). In order to avoid such unrealistic realization of onset and demise dates, we first
stipulate that onset may not occur during the last three months (i.e. 92 days) of the year.
Second, we stipulate that the demise must occur after the onset. As an extreme example,
daily AIR and its corresponding cumulative daily anomaly for the year 1972 are shown in
Fig. 4. This year experienced the most severe drought of the ISM since the beginning of the
11
20th Century, and is often referred to as the Maharashtra Drought of 1972 (Bhat, 2002). It is
apparent from the figure that without the second stipulation, one would have determined an
unrealistic demise date for this season. Note that this is the only year from 1902-2005 during
which these stipulations were necessary. Taking these stipulations into account, the onset of
the ISM is defined as the day after the cumulative daily anomaly of AIR reaches absolute
minimum before the last three months of the year. Similarly, the demise of the ISM is defined
as the day when the cumulative daily anomaly of the AIR reaches absolute maximum after
the onset date. This index is henceforth referred to as the All-India rainfall onset and demise
(AIROD). One may refer to only the onset or demise component of the index as AIRO or AIRD,
respectively.
3.2 Insensitivity to False Onsets
The AIRO must be insensitive to false onsets caused by synoptic disturbances to be
considered an effective onset index. Multiple case studies are presented alongside one
another to determine its effectiveness at bypassing temporary bouts of heavy rainfall and
detecting the actual onset date. Seasonal cycles of daily AIR and its cumulative anomalies
are analyzed for the following eleven false onset years: 1946, 1958, 1967, 1968, 1972, 1979,
1986, 1995, 1997, 2002, and 2004 (Table 4). These years are selected from previous research
devoted to the subject of false onsets which verifies such occurrences with various methods.
Fieux and Stommel (1977) seem to have first introduced the term “multiple onset,” and
detected four false onset years – 1946, 1958, 1967, and 1968 – from the period between 1933
and 1968 using southwesterly surface winds from shipping data over the Arabian Sea. These
false onsets were characterized by an episodic increase followed by an immediate decrease of
the southwesterly winds. Most of the other false onset years are taken from Flatau et al.
(2001), who use three criteria to determine such an event from 1965 to 1997: 1) kinetic energy
12
of the surface winds averaged over 5-20N and 40-110E (similar to Fieux and Stommel,
1977); 2) shear between 850hPa and 200hPa zonal winds averaged over 5-20N and 40-
110E (Webster and Yang, 1992); and 3) shear between 850hPa and 200hPa meridional
winds, averaged over 10-30N and 70-110E (Goswami et al., 1999). These three criteria
are all met for 1967, 1972, 1979, 1995, and 1997. The year of 1986 fulfilled only the first two
criteria, and the year of 1968 only satisfied the first but is also supported by Fieux and
Stommel’s (1977) observations. Similarly, Flatau et al. (2003) implements the first and third
criteria from their previous paper to include 2002 as a false onset year. The final year
analyzed, 2004, is indicated as a false onset year by Pai and Rajeevan (2009), who describes
it as a synoptically triggered event similar to that of 2002.
Three dates are compared for each case year’s seasonal cycle: the false onset, the
“actual onset,” and the AIRO (Table 4). False onset dates for the first four cases – 1946, 1958,
1967, and 1968 – are provided by Fieux and Stommel (1977): 12 May, 10 May, 17 May, and
5 May, respectively. The following five years – 1972, 1979, 1986, 1995, and 1997 – are more
ambiguous because Flatau et al. (2001) does not provide specific false onset dates as each of
their three criteria would offer different solutions. The false onset date for 1972 is ascertained
from NPTEL (2013) as 16 May. For the four other years, the date of false onset is selected
following Flatau et al. (2001) as the day when “the initial convective perturbation lead to the
development of the twin convective systems straddling the equator near 80-90E”. The onset
dates for the monsoon seasons of 1979, 1986, 1995, and 1997 are 9 May, 10 May, 9 May, and
14 May, respectively (Fig. 5). Furthermore, Flatau et al. (2003) and NPTEL (2013) suggest a
false onset date of 29 May and 18 May for 2002 and 2004, respectively.
The IMD subjective onset definition (Ananthakrishnan and Soman, 1988) is
considered to be the “actual” onset over Kerala against which the AIRO date will be compared
13
through 1970. This definition takes into account persistently heavy daily rainfall for rain
gauges, strength and depth of lower tropospheric westerly winds, and high relative humidity
up to at least 500hPa all over Kerala (Rao, 1976). From 1971 to 2005, an objective onset
definition adopted by the IMD in 2006 is considered to be the “actual” onset over Kerala, as
the objective definition is applied without a forecaster’s bias (Pai and Rajeevan, 2009). This
definition has three criteria, but emphasis is given to the first:
1. If after 10 May, 60% of the available 14 stations in Kerala report rainfall of 2.5 mm
or more for two consecutive days, the onset may be declared on the second day,
provided the following criteria are also satisfied in concurrence.
2. Depth of westerlies should be maintained up to 600hPa, from the equator to 10°N and
55° to 80°E. The zonal wind speed over the area bounded by 5° to 10°N, 70° to 80°E
should be 15-20 knots at 925hPa.
3. Outgoing longwave radiation should be below 20Wm-2 from 5° to 10°N and 70° to 75°E.
It may be noted, however, that AIRO dates and “actual” onset dates may differ due to
difference in domain. This is not a weakness of either method, but rather represents their
different objectives. Also, as is attested to by numerous articles (Flatau et al., 2001, 2003;
NPTEL, 2013), the IMD sometimes declares the onset of the ISM prematurely by using the
criteria of their Kerala onset definitions, but adjusts its forecast after a failed attempt to
match the timing of actual onset for recording purposes. This adjustment to the actual onset
each year is the reason for our confidence in treating the IMD onset definitions as providing
“actual” onsets and verifying the timing of AIRO dates accordingly.
3.3 Seasonal Evolution
At this point, it is possible to determine the seasonal evolution of three general
categories of variables that exhibit significant changes during the onset and demise of the
14
ISM: rainfall, from which the AIR transition dates are derived; large-scale atmospheric
phenomena; and large-scale oceanic phenomena. Using rainfall as a preliminary example,
gridded and spatially averaged composite analyses of rainfall centered on onset are
calculated and plotted to examine its climatological progression. The composite is created by
calculating the rainfall for a specific day relative to each year’s onset date. The average of
that day’s values is then computed. This process is repeated for as many days leading and
lagging the onset as desired; in this study, as many as 120 days preceding and succeeding
onset are plotted. The gridded composite analysis is depicted as a spatial map for each pentad
leading and following onset, while every day is graphed on a line plot for the spatially
averaged composite analysis. An identical composite analysis is performed centered upon
demise date. Only a maximum of sixty days before and after demise are plotted, however, as
there are some cases when demise date is very nearly two months from the final day of a
particular year, and adding any more lagging days would result in sampling from the
following year.
A plethora of atmospheric variables besides rainfall are analyzed in this study to
provide a comprehensive characterization of the AIROD (Table 5). As discussed in the
introduction, these variables have also been used to characterize the onset and demise of the
ISM in earlier studies. Comparing these variables with our index of onset and demise
therefore provides a context to its efficacy. These six variables (some of which are derived
from others) include precipitable water, vertically integrated moisture flux convergence,
300hPa temperature, another temperature-derived variable, and two additional variables
derived from the zonal and meridional components of wind at 850hPa and 200hPa.
Precipitable water is the depth of water in a column of the atmosphere if all the water
in that column were precipitated as rain and is directly obtained from atmospheric reanalysis
ERA-20C. Similarly, vertically integrated moisture flux convergence is the convergence of
15
water in a column of the atmosphere and is derived from the atmospheric reanalysis. 300hPa
temperature is also obtained directly from the atmospheric reanalysis. From this metric, the
meridional temperature gradient between 5N and 25N is computed. Lastly, zonal and
meridional components of the wind field at 850hPa and 200hPa are obtained from the
atmospheric reanalysis and are used to derive two final variables of interest. One of these
two variables is the kinetic energy of the wind at 850hPa, which is calculated with this
equation: � = + , (3)
where and are respectively the zonal and meridional components of wind. The other
metric derived from the wind field is the magnitude of vertical wind shear between 850hPa
and 200hPa. Vertical wind shear is computed in this manner: = √ ℎ�� − 85 ℎ�� + ℎ�� − 85 ℎ�� . (4)
Three oceanic are analyzed in addition to the aforementioned atmospheric variables,
to characterize the AIROD (Table 5). First, zonally-averaged meridional ocean heat
transport, or the amount of heat transported across a particular latitudinal band in the ocean,
is a function of potential temperature and the meridional component of current velocity. The
zonal component of ocean heat transport is neglected because it is much less homogeneous
across the Indian Ocean and the progression of its reversal is much less consistent. In this
study, meridional heat transport is zonally-averaged for 0.5° increments from one coast of
the Indian Ocean to another at each latitude. The equation for zonally-averaged meridional
heat transport is given as �� = ���� ∬ �� � , (5)
where is meridional current velocity, � is potential temperature, and respectively
represent longitude and depth, is the number of longitudinal grid points over which it is
16
averaged, is the specific heat capacity of sea water (3993Jkg-1K-1), and � is the density of
sea water (1024kgm-3; NPL, 2016). Although density and temperature of sea water does
change with depth, these changes have minimal effect on the calculation of meridional heat
transport to roughly 500 meters below the surface. The depth of integration is 105 meters (11
levels). Although Loschnigg and Webster’s (2000) studies integrated to a depth of 500m, 105
meters is considered a clearer representation of meridional heat transport for a few reasons.
First, the Indian Ocean mixed layer depth is roughly 50 to 100 meters depending on season
and latitude (Montegut et al., 2004). As a result, recent research constrains itself to this layer
when computing meridional heat transport (Baquero-Bernal et al., 2002; Sun et al., 2014).
Going deeper than about 100 meters may result in sampling currents that flow in opposite
directions and thus provide weaker depth-accumulated current speed than exists in the
mixed layer. These weaker currents would in turn weaken the signal of meridional heat
transport in the ocean. The second oceanic metric is monthly averaged sea surface
temperatures (SST) and is compared to the AIROD dates to locate any teleconnections that
may exist. A final and rather similar metric, Niño 3.4 SST, is analyzed to determine the
relationship of various ISM features to the El Niño–Southern Oscillation (ENSO).
3.4 Interannual Variability
The interannual variability of AIROD dates effect how large-scale phenomena evolve.
That is, a particular atmospheric or oceanic feature may show a significant difference in
behavior between years with early and late AIROD dates. This variability is analyzed in a
similar manner as seasonal evolution.
The first task in computing correlations is to determine if trends in the ISM features
are significant enough to account for. Both linear trends and ten-year moving averages of
17
AIRO date, AIRD date, and AIR-based season length are computed and analyzed (Fig. 6).
None of these ISM features show a statistically significant linear trend when tested at the
5% significance level using the Mann-Kendall significance test (Sneyers, 1990). A major
reason for the insignificant linear trends is because the annual mean AIR also shows an
insignificant linear trend (Fig. 6d). Therefore, trends are not removed from any of these
features of the ISM before other calculations are performed.
The distribution of AIRO date, AIRD date, and AIR-based season length, are
calculated next to determine whether they are Gaussian. As Fig. 7 reveals, none of the three
parameters are Gaussian. Onset dates are negatively skewed and contain two notable
maxima, while season lengths are positively skewed. Demise dates also display two maxima
unlike a Gaussian distribution.
Many features of the ISM are then compared over the 104 years to one another and
to large-scale atmospheric and oceanic phenomena using the sample Pearson correlation
coefficient (referred to simply as the correlation coefficient in many studies): � = ∑ � �− ̅ ̅√(∑ �2− ̅2)√(∑ �2− ̅2), (6)
where and are two variables, ̅ and ̅ are the variables’ means, � is the year, and is the
number of years. Essentially, the correlation coefficient is the covariance of the two variables
divided by the product of their standard deviations. The coefficient’s significance is tested
using the iterated bootstrap method (Efron, 1979; Chernick, 2008; Wilkes, 2011). The
distributions are dissimilar to a Gaussian, or normal, distribution and there is a relatively
large sample size of 104 values (Fig. 8), so this method is used instead of a student t-test or
other similar significance test because it does not need to assume normality (DiCiccio and
Efron, 1996). The null hypothesis to be tested is that the correlation computed for a pair of
variables may be randomly produced. First, the correlation for a pair of non-Gaussian
18
variables (e.g., 104 onset dates and AIR quantities for the years 1902 to 2005) is computed.
Next, the values for one of the two variables are randomly reordered to obtain a new
combination of pairs known as a bootstrap sample, and this sample’s correlation is computed.
This method of resampling (i.e. the Monte Carlo method; Hall, 1992) and subsequent
correlation are repeated for a sufficient number of iterations (e.g., 1,000 iterations are
recommended by Efron (1987) for hypothesis testing). The variance of each variable is
retained by this resampling technique, so this significance test is testing for the significance
of the covariance only. The distribution of the sample correlations is then determined by
ordering them from least to greatest. Finally, a confidence interval is selected (e.g., 95%). If
the original sample’s correlation falls outside of the confidence interval (e.g., smaller than
2.5% or greater than 97.5% of the bootstrap samples’ correlations), then the null hypothesis
is rejected (i.e. the correlation is considered to be significant and is highly unlikely to be
randomly producedChernick, 2008). All correlations computed in this study (with the
exception of those involving Niño 3.4 SSTs) are tested for significance using the iterated
bootstrap method at the 5% significance level for 1,000 bootstrap samples.
19
CHAPTER 4
RESULTS AND DISCUSSION
4.1 Insensitivity to Arbitrary Domain Changes, Time Period Changes, and False Onsets
In order to ensure that the AIROD is insensitive to arbitrary changes in domain (e.g.,
political boundaries), a new domain is tested that includes the adjacent nation of Bangladesh.
The APHRODITE rainfall dataset (Yatagai et al, 2012) is used to accomplish this objective,
as the ground stations used over the Indian subcontinent are identical to those in the AIR
dataset albeit for a shorter period from 1951 to 2005. A square gridded region is selected from
21.25 to 26.25N and from 88 to 92.5E that encompasses the political border of Bangladesh,
and APHRODITE data within this region and the predefined IMD Indian region are
combined to form the new domain which will henceforth be referred to as APHRO (Fig. 9).
Finally, the rainfall within the APHRO domain provides a new set of onset and demise dates,
and these dates are compared with the AIROD dates which are recomputed for the years
1951 to 2005.
The APHRO onset and demise dates do not differ significantly from AIROD dates for
the years 1951 to 2005 (Fig. 10). The climatological AIR onset and demise dates for this time
period are 5 June and 7 October, respectively. Climatological APHRO onset and demise date
departed from AIROD dates by less than a day, being respectively 4 June and 7 October when
rounded to the nearest day. The two domains’ minimum and maximum onset and demise
dates also diverge by less than one day with the exception of the maximum APHRO demise
date, which ends eight days before the AIR demise date. This difference is due to the earlier
withdrawal of rainfall from the northeastern portion of each domain. Therefore, it is
reasonable to conclude that changes in domain due to inclusion of nearby countries or
20
changes in political boundaries do not greatly influence the onset and demise dates of the
ISM.
The AIROD is directly related to the climatological annual mean, a single threshold
value that is determined by the average of the annual means of a sample of years. It is
possible that the number of years, or even the particular era sampled, can alter the onset and
demise significantly. The annual mean rainfall ranges from 2.50mm to 3.79mm, with a
standard deviation of 0.27mm. No significant departure from the climatological annual mean
occurs for fifteen-year averages and greater. However, five- to ten-year averages are
inadequate in some eras for calculating the climatological annual mean and fall outside of a
standard deviation from the 104-year climatological annual mean implemented in this study
(Fig. 6d). Therefore, one may safely use the AIROD for a period of fifteen years or more
without significantly altering the onset and demise dates.
Not only should the AIRO be insensitive to minor changes in domain and changes in
time period, but it must also be insensitive to false onsets caused by synoptic scale
disturbances. The AIRO effectively bypasses every historical case of false onset and indicates
a date that falls within a few days of onset determined by IMD for Kerala (Fig. 11;
Ananthakrishnan and Soman, 1988; Pai and Rajeevan, 2009). Refer to section 3.2 for an
explanation of why this onset definition is considered “actual”. The AIRO occurs about one
month after the false onset, a result which closely coincides with the pre-monsoon rainfall
peak observed by Joseph and Pillai (1988). It is therefore safe to conclude that the AIRO is
insensitive to false onsets.
4.2 Seasonal Evolution
Much is understood concerning the physical mechanisms involved in initiating the
ISM. Land surfaces have a lower heat capacity than oceans, and only conduction occurs in
21
soil whereas heat is dispersed through both conduction and convection in water. This
difference allows for more rapid heating (or cooling in the absence of a heat source) over land
than over water. The land is therefore much colder in boreal winter due to radiative cooling
compared to oceans which retain some of the previous summer’s radiation. As spring gives
way to summer, incoming solar radiation intensifies at increasingly higher latitudes. Not
only are there large land masses farther north of the equator, but the Tibetan Plateau is a
location of very high altitude. Since the atmosphere becomes cooler at higher altitudes, but
land effectively heats (cools) the overlying atmospheric column in the presence (absence) of
solar radiation, this plateau acts as an elevated heat source during the summer (Wu and
Zhang, 1998). At a certain point during the year, the meridional temperature gradient
produced by the land-ocean temperature contrast and exacerbated by the Tibetan Plateau
reverses sign, becoming negative instead of positive (Yanai et al., 1992; Hsu et al., 1999).
As the atmosphere above land experiences anomalous heating relative to that above
ocean, the atmospheric column expands and its density decreases as mass is displaced by
divergence at the tropopause. This tropospheric expansion and contemporaneous upper-level
divergence results in an anomalously low surface pressure over the Indian subcontinent. The
pressure gradient between the land and the surrounding ocean increases and is partially
offset by the Coriolis, centrifugal, and viscous forces that slow incoming winds and turn them
to the right in the Northern Hemisphere. Therefore, winds flow cyclonically inward to
equalize the pressure difference and restore the force imbalance (Rao, 1976; Hsu et al, 1999).
Prior to onset, low-level wind near the equator is westerly in the Southern
Hemisphere and easterly in the Northern Hemisphere. The aforementioned large-scale
cyclonic circulation over the Indian subcontinent in combination with counterclockwise
rotation about the Mascarene High in the Southern Hemisphere cause the low-level wind
direction near the equator in both hemispheres to reverse and intensify, especially off the
22
Somali coast (Rao, 1976; Webster and Yan, 1992; Soman and Kumar, 1993; Lau et al., 1998;
Goswami et al., 1999; Hsu et al., 1999). The ocean currents averaged over the mixed layer of
the ocean, known as the Ekman current, flow to the right (left) of the surface wind in the
Northern (Southern) Hemisphere due to the influence of the wind-induced stress at the
surface and the competing Coriolis and turbulent drag forces at various depths (Fig. 12;
Ekman, 1905). Therefore, a reversal of wind across the Indian Ocean forces a basin-wide
reversal of the Ekman current and its related heat transport (Fig. 13; Loschnigg and Webster,
2000).
Frictional convergence occurs as moisture-laden surface winds transition from the
lower-friction Arabian Sea and Bay of Bengal to the rougher land surface of the southern tip
and northeastern region of the Indian subcontinent, hence contributing to excess moisture
over Kerala and the seven sister states (Fig. 1). Numerous processes assists this surplus of
precipitable moisture. Diabatic heating over land increases buoyancy and causes mixing of
warm, dry air above the land with cooler, moist air from the ocean (Hsu et al., 1999). This
convergent air is then orographically lifted on the windward side of the Western Ghats
mountain range in the south and the Himalayan Mountains in the northeast. This sudden
availability of instability, moisture, and lift results in deep moist convection and intense
rainfall over Kerala and the seven sister states (Ananthakrishnan and Soman, 1988; Soman
and Kumar, 1993; Lau et al., 1998; Goswami and Gouda, 2010). Meanwhile, a more steady
increase in precipitation takes place in central India as moisture converges due to the large-
scale cyclonic circulation previously discussed.
It is clear that a seasonally varying land-ocean temperature contrast influences large-
scale atmospheric circulations, which in turn reverses oceanic circulations and results in
sudden and severe regional precipitation. The AIROD captures the seasonal evolution of
23
these large-scale atmospheric and oceanic processes and in so doing reveals its intrinsic
relationship with the physical mechanisms that initiate the onset and demise of the ISM.
4.2.1 The Land-Ocean Temperature Contrast
Increased heating of the Tibetan Plateau and, to a lesser extent, the entire continental
landmass is evident leading up to the onset of the ISM (Wu and Zhang, 1998). An increase of
300hPa temperature first begins in the East Asian monsoon region and the Bay of Bengal a
month before the onset of the ISM. Roughly five days before the AIRO, intensified heating
over the region surrounding the seven sister states expands to the east and west, resulting
in higher temperatures to the north than nearer the equator (Fig. 14). This relatively high
northerly upper level temperature persists until about twenty days before the AIRD when it
begins to contract towards the Himalayan foothills and withdraw to the southeast (Fig. 15).
This robust seasonal feature of the ISM evolution may be more clearly and simply
depicted by the seasonal reversal of a rather strong meridional temperature gradient at
around 300hPa. Yanai (1992) notes a reversal of this meridional temperature gradient
between 5°N and 25°N, which is generally negative prior to onset and reverses to a positive
value after the ISM is established. The AIROD captures this feature very well (Fig. 16), with
the reversal of the temperature gradient (i.e. the intersection with the zero contour line)
occurring about twenty days before the AIRO in the eastern longitudes of the East Asian
monsoon (east of 90°E). This reversal steadily progresses westward, reaching 60°E at the
time of the AIRO and then continuing west (Fig. 16a). Similarly, the reversal of this
meridional temperature gradient begins previous to the AIRD west of 60°E and afterwards
continues further eastward to almost 110°E (Fig. 16b). Examining upper level temperature
and its gradient from south to north in the context of the AIROD reveals an adequate
representation of the land-ocean temperature contrast that leads to the ISM.
24
4.2.2 Large-Scale Atmospheric Circulation Reversal
The reversal of low-level winds off the Somali coast is of paramount importance to
accurately represent as the monsoon is technically defined by this seasonal shift of prevailing
wind direction. Upper and lower level winds, and their combined vertical wind shear, reverse
and intensify around the time of the onset of the ISM (Webster and Yang, 1992; Lau et al.,
1998; Goswami et al., 1999; Hsu et al., 1999). Fig. 17 displays constantly vigorous 850hPa to
200hPa vertical wind shear in the midlatitudes as a result of the upper level jetstream that
shifts further north as the AIRO approaches. What is of most importance concerning the
mechanisms associated with the AIRO, however, is the growth of vertical wind shear in the
typically shearless tropical environment. This shear first begins to develop in the southern
Bay of Bengal about fifteen days before the AIRO, and by the AIRO the vertical wind shear
over the southern Arabian Sea off the coast of Somalia doubles in magnitude (Fig. 17). This
vertical wind shear continues to intensify and extend toward the Indian peninsula as the
ISM progresses until a little over a month before the AIRD. By the AIRD, vertical wind shear
is weakened and its attendant winds are weakened in the tropics, while the upper level
jetstream in the midlatitudes intensifies and shifts further south as boreal winter approaches
(Fig. 18).
Kinetic energy of 850hPa winds dramatically increase as a direct consequence of the
reversal and subsequent increase of low-level winds (Krishnamurti and Ramanathan, 1982).
Krishnamurti and Ramanathan (1982) observes more than an order of magnitude increase
in zonal kinetic energy over a period of a week for the year 1979 from 50° to 70°E and 4°S to
20°N. A 104-year composite analysis does not show as drastic a change (Figs. 19 and 20). This
suggests that the year 1979 had an anomalously large increase in kinetic energy and that
such limited sampling improperly magnified the expected magnitude of increase in low-level
kinetic energy. A new region of interest is selected from 50 to 75° and 5 to 20°N to most
25
adequately represent the changes in total kinetic energy of 850hPa winds during the seasonal
evolution of the ISM. Prior to onset, kinetic energy is marginal and remains below 75m2s-2.
Kinetic energy suddenly doubles during onset to 150m2s-2, and then doubles again as the ISM
progresses (Fig. 19). Kinetic energy changes more slowly during withdrawal of the ISM, and
by the AIRD has decreased to less than 50m2s-2 (Fig. 20). Thus, while the increase in low-
level kinetic energy is not as dramatic as is anticipated by previous studies, its evolution
remains quite sudden and its characteristics are clear. These two wind-based variables show
that the AIROD captures the reversal and subsequent intensification of the atmospheric
circulation well.
4.2.3 Large-Scale Oceanic Circulation Reversal
A reversal in Ekman heat transport in the Indian Ocean accompanies the reversal in
atmospheric circulation preceding the onset of the ISM. Loschnigg and Webster (2000) notes
such a dramatic reversal from northward to southward Ekman heat transport that it roughly
balances the northward atmospheric heat transport. The pattern of reversal of basin-wide,
zonally-averaged meridional ocean heat transport given in previous literature (Chirokova
and Webster, 2006) is replicated by the AIROD (Fig. 21). Below about 15°S, meridional heat
transport remains southward throughout most of the year. The reversal from northward to
southward meridional heat transport begins at about 12°S, and this reversal rapidly
propagates northward about twenty to forty days before the AIRO up to around 10°N. The
most sudden reversal and subsequent intensification of southward transport seems to take
place here, and by the AIRO southward heat transport is occurring at all but the most
northern latitudes of the Indian Ocean (Fig. 21a). Within roughly three months, meridional
heat transport once again reverse from southward to northward transport, beginning in the
26
northern latitudes and reaching 10°N by the AIRD. This reversal continues at a slower rate
into the Southern Hemisphere after the AIRD (Fig. 21b).
A few interesting characteristics of meridional ocean heat transport should be
mentioned. First, 10° to 15°S experiences the greatest southward heat transport in the
southern portion of the Indian Ocean, which is in agreement with previous research
(Chirokova and Webster, 2006; Sun et al., 2014). There exists the most sudden and strong
gradient in meridional heat transport at about 8° to 10°N, where reversal occurs a little less
than twenty days before the AIRO. Both of these are two examples of the multiple striations
in meridional heat transport apparent throughout the Indian Ocean (Fig. 21). This
inhomogeneous transport results from the competition between boundary currents and the
basin-wide Ekman transport. Higher values of meridional heat transport are observed, as
stated above at 10° to 15°S and 8° to 10°N. The former is the latitudinal domain of the
Mozambique and Southeast Madagascar Currents, which continually flow to the south. The
latter is the location of the Great Whirl which produces roughly balanced meridional
transport (Beal and Donohue, 2013, Akuetevi et al., 2016). These phenomena, especially the
currents to the south, positively reinforce the basin-wide southward Ekman transport
immediately before and during the ISM, thus generating greater southward meridional heat
transport. Conversely, the East African Coastal Current (around 10°S to the equator) flows
consistently northward throughout the year, thus opposing basin-wide Ekman transport
preceding and during the ISM and causing weaker southward meridional heat transport (Fig.
21a). The Somali Current is unique in that it is the only ocean current that experiences an
annual reversal, flowing northward in the boreal summer and southward in the boreal winter
(Beal and Donohue, 2013). This current opposes the flow of Ekman transport before, during,
and after the ISM, therefore weakening southward meridional heat transport during the ISM
and weakening northward meridional heat transport at other times of the year (Fig. 21a). All
27
of these interactions appear during the seasonal evolution of meridional heat transport based
on the AIROD.
Another interesting characteristic of meridional heat transport is the diagonal lines
of alternating maximum and minimum transport across the equator (Fig. 21). This
phenomena is explained by the Rossby duct hypothesis (Sahami, 2003). Pairs of Rossby waves
straddling the equator form a wave train between the southward Ekman transport that
begins at roughly 6°S and 6°N. Ekman transport becomes infinitesimal near the equator as
the Coriolis force weakens and ultimately reverses. The Rossby wave structures that span
this equatorial region where Ekman flow is no longer valid allow continuous flow across the
equator through the ducts displayed in Fig. 22. The southward flow within the antisymmetric
structure of the waves is enhanced by the steady southward flow which overlaps the poleward
edges of the equatorial wave guide, thus resulting in regions of enhanced southward heat
transport near the equator (Figs. 21 and 22; Sahami, 2003).
Finally, for reasons that are unclear, this study’s values are almost exactly an order
of magnitude smaller than that of previous studies (a maximum of 0.3PW compared to a
maximum of 2.5PW) despite the pattern of meridional heat transport being nearly identical
(Chirokova and Webster, 2006). This discrepancy may not be attributed to the influence of
boundary currents because separate calculations were completed excluding the boundary
which obtained similar magnitudes. Furthermore, the problem is not a result of spatial
resolution, since a recent research with 0.5° resolution (identical to this study) derives similar
values as previous research (Sun et al., 2014). It is possible that either CFSR or other models
(e.g., two-and-a-half-layer Indian Ocean model; SODA) are unable to accurately resolve the
strength of ocean currents and therefore inadequately represent meridional heat transport.
This seems unlikely, however, given the striking similarity in the pattern of meridional heat
transport between the different models. Other reasons for the difference in magnitude
28
include the difference in time step or the difference in depth over which transport is
integrated. Chirokova and Webster (2006) compute meridional heat transport in five-day
intervals, which is insufficient for determining the date of onset and may lead to different
values than the previous study. A difference as drastic as an order of magnitude, however,
could not result from this difference in time step. Previous research integrates over the top
500 meters (Chirokova and Webster, 2006) or entire depth (Sun et al., 2014) of the Indian
Ocean, whereas the current study only integrates the top 105 meters known as the mixed
layer. Deeper sampling could result in an increase in meridional heat transport (i.e.
additional layers provides a greater value) or, if too deep, a potential decrease in transport
(i.e. opposing undercurrents are also included in integration). That said, multiple depths
were attempted in this study that altered the pattern of the meridional heat transport more
than its magnitude. In conclusion, while meridional heat transport seems to provide advance
warning for the AIROD, it must be further scrutinized to understand the discrepancies
involved.
4.2.4 Moisture Convergence and Subsequent Precipitation
The AIROD is based upon rainfall, so it is expected and of highest priority that the
seasonal evolution of moisture-based variables are well represented. Vertically integrated
moisture flux convergence begins to increase in an arc to the south and east of the Indian
subcontinent about fifteen days prior to the AIRO due to the large-scale cyclonic circulation
about the landmass. Meanwhile, divergence exists over the central Arabian Sea and southern
India. By the AIRO, frictional convergence over the southern tip of India and over the seven
sister states generates a maximum in moisture convergence. This convergence arises from
the shift from relatively frictionless ocean to the rough land surface and mountain ranges.
About fifteen days later, large-scale convergence causes moisture to congregate over central
29
India (Fig. 23). This moisture convergence persists only over the Himalayan foothills by the
AIRD, at which point there is widespread divergence over land and convergence over the Bay
of Bengal and the South China Sea (Fig. 24). This southwestward withdrawal of moisture
provides the environmental setup necessary for the Australian monsoon.
A similar evolution may be seen for precipitable water. Moderate values (45-50kgm-2)
reside only in the southern Bay of Bengal about a month before the AIRO. These moderate
values then begin to expand and increase, first over far eastern Asia, followed by the northern
Arabian Sea and finally over the southern Arabian Sea and the seven sister states to the
north. At AIRO, precipitable water dramatically intensifies discreetly at the coast of Kerala
and over the seven sister states. After onset, high values (55-60kgm-2) of precipitable water
progress over central India, with the highest values (60-65kgm-2) remaining over the
Himalayan foothills (Fig. 25). As the AIRD approaches, higher values of precipitable water
withdraw eastward and are constrained to the Bay of Bengal (Fig. 26). This evolution is
nearly identical to vertically integrated moisture flux convergence since a convergence of
moisture leads to a localized higher concentration of moisture, or precipitable water. The rain
shadow to the east of the Western Ghats in southern India (which is also captured in rainfall
composites) is more clearly visible as a minimum in precipitable water, however (Fig. 25).
The most dramatic change captured by the AIROD is that of gridded rainfall. The
Indian subcontinent is devoid of even light (2-10mmday-1) rainfall except for over the seven
sister states, which are influenced by the Asian monsoon and thus exhibit a rather steady
moderate (10-20mmday-1) rainfall up to two months in advance of the AIRO. On the AIRO
date, rainfall dramatically increases (20-30mmday-1) in Kerala and the seven sister states
with a light (2-8mm) increase beginning in south and east India. As the ISM progresses,
central India sees a major increase (10-20mmday-1) in rainfall that then extends to the
northwest. Meanwhile, the seen sister states, and to a greater extent the southwest Indian
30
coast, experience severe (>30mmday-1) rainfall (Fig. 27). This heavy precipitation across the
Indian subcontinent persists until about 45 days before the AIRD when rainfall begins to
slowly weaken in all regions. Withdrawal begins in the northeast about 25 days before the
AIRD. This gradual withdrawal and weakening precipitation abruptly accelerates
immediately before the AIRD, leaving only light (2-10mm) rainfall in India. This rainfall
slightly increases within a few days and persists in southeast India for at least two months
as the Indian winter monsoon arrives (Fig. 28).
4.3 Interannual Variability
The AIROD has been shown to adequately represent the seasonal evolution of the ISM
and changes in its related large-scale atmospheric and oceanic phenomena. The interannual
variability of the AIROD and its associated large-scale variables is assessed to determine
how one varies with respect to the other. Possible causal relationships are also discussed by
using the physical mechanisms observed during the seasonal evolution previously presented
and using lead and lag relationships.
4.3.1 Features of the Indian Summer Monsoon
Before analyzing the interannual variability of large-scale atmospheric and oceanic
variables, one must understand how certain ISM features are interrelated. Five features are
of particular interest: AIRO, AIRD, season length, total seasonal AIR, and mean seasonal
AIR. While the AIRO and AIRD are not significantly correlated with each other (-0.12), both
are highly correlated with season length (-0.67 and 0.82, respectively; Table 6). This
relationship indicates that an early (late) AIRO date and a late (early) AIRD date by
definition result in a longer (shorter) length of the ISM. Furthermore, the AIRO and AIRD
are well correlated with total seasonal AIR (-0.43 and 0.61, respectively), showing that an
31
early (late) AIRO date and a late (early) AIRD date also result in greater seasonal rainfall
averaged over India (Table 6). This could be a direct result of increased season length, or of
increased rain rate at the beginning or end of the ISM. However, the sign of correlation
coefficient switches for the AIRO and AIRD with mean seasonal AIR (0.27 and -0.24,
respectively) compared to total seasonal AIR, which insinuates that the effect of season
length on total seasonal AIR is more significant than that of rain rate (Tables 6 and 7).
Caution is recommended in interpretation of these correlations, however, as it is possible that
cross-correlation has caused inappropriate inflation of values. This effect could arise from the
inherent noisiness of rainfall data, but cannot be removed from results due to the difficult
task of distinguishing noise from annual variability.
Total seasonal rainfall variability dominates in different locations for changes in
AIRO date and AIRD date. An early (late) AIRO date suggests a higher probability (� � =− . ) of increased (decreased) seasonal rainfall particularly in the seven sister states,
although central and southern India also weakly retain this relationship (Fig. 29a). A late
(early) AIRD date, on the other hand, suggests an even greater probability (� � = . ) of
increased (decreased) seasonal rainfall predominantly in southeast India, but to a lesser
extent throughout the remainder of the Indian subcontinent (Fig. 29b). The reason for this
discrepancy of location of increased seasonal rainfall is rather simple. An early AIRO date
implies an increase in rainfall compared to climatology near the beginning of the season, and
the opposite may also be argued concerning a late AIRO date. ISM rainfall commences over
Kerala and the seven sister states, so this early-season anomalous rainfall should influence
the total seasonal rainfall most greatly in these regions. Likewise, ISM rainfall reaches its
final point of withdrawal in southeast India, so a late (early) AIRD date should result in
32
increased (decreased) late-season rainfall relative to climatology and consequently increased
(decreased) total seasonal rainfall at this location.
4.3.2 Temperature
Upper level temperature anomalies vary as the timing of the AIROD changes. The
300hPa meridional temperature gradient between 5°N and 25°N reveals a significantly
negative correlation (� � = − . ) from 40°E to 70°E beginning fifteen days before the AIRO
that extends eastward to 90°E at AIRO and persists for another twenty days (Fig. 30a). That
is, an early (late) AIRO date is associated with an increased (decreased) meridional
temperature gradient anomaly relative to climatological values fifteen days before to twenty
days afterwards. An inverse relationship exists between the AIRD and the upper level
meridional temperature gradient (� � = . ), with an early (late) AIRD date often
associated with a decreased (increased) meridional temperature gradient anomaly beginning
five days before at about 80°E and continuing until about five days afterwards at about 60°E
(Fig. 30b). A climatologically anomalous meridional temperature gradient observed to persist
for roughly ten to fifteen days may indicate the timing of the AIRO.
The zonal progression of this anomaly of temperature difference between latitudes
can be further explored by observing the spatial relationship between the AIROD and 300hPa
temperature itself. The anomalous increase (decrease) in upper level temperature begins
about ten days prior to an early (late) AIRO over the Arabian and Thar deserts to the west,
and then slowly progresses across the Arabian Sea and into northern India five days after
the AIRO (Fig. 31). The opposite progression of temperature anomalies takes place at the end
of the ISM, with AIRD date anomalies positively correlated with temperature anomalies five
days before over northern India to five days after over the western deserts (Fig. 32). It should
33
be noted that while the maximum upper level temperatures occur in northeast India (Fig.
14), the anomalous relationship indicating the arrival of the AIROD is far west of this
maximum.
4.3.3 Wind
Less can be said about the relationship between 850hPa to 200hPa vertical wind shear
and the AIROD because of the noisiness of observations of vertical wind shear and the
possibly strong influence of intraseasonal variability contaminating the analysis. This
noisiness may in part be a result of sampling 200hPa winds, which are not represented with
great accuracy by the surface-assimilated ERA-20C (Poli et al., 2013). However, a general
conclusion can be made that an early (late) AIRO date would occur shortly after an early
(late) establishment of the large-scale atmospheric circulation about the Indian subcontinent.
This relationship is manifested as negative correlations (� � = − . ) extending across the
Indian Ocean at the southern tip of the subcontinent and positive correlations (� � = . )
extending across northern India and the bordering nations around the AIRO (Fig. 33). These
correlations then flip signs in the days before and after the AIRD (Fig. 34), insinuating that
an early (late) AIRD date corresponds to an early (late) withdrawal of the large-scale
atmospheric circulation about the Indian subcontinent.
The variability of kinetic energy of 850hPa winds, however, is more clearly related to
the timing of the AIROD. Beginning fifteen days before the AIRO, there appears an
anomalous increase (decrease) in low-level kinetic energy off the Somali Coast for an early
(late) AIRO date (� � = − . ). As the AIRO approaches, this anomaly shifts eastward across
the Arabian Sea, all the while remaining centered just north of 10°N (Fig. 35). A rather
similar process develops during and after the AIRD, with a positive correlation (� � = . )
34
centered just south of 10°N and slowly progressing westward across the Arabian Sea (Fig.
36). This variability of the kinetic energy is useful to monitor as it exhibits a highly
concentrated and easily recognized anomaly well in advance of the AIRO.
4.3.4 Oceanic Phenomena
Not much may be deduced from the correlation of AIROD dates with meridional ocean
heat transport (Fig. 37). The noisiness and wave-like patterns may be result of the slow
response of the ocean compared to the atmosphere and the production of westward-
propagating Rossby waves. Due to these complications, no reasonable conclusions may be
drawn from this relationship.
Teleconnections exist between AIRO date variability and the preceding December-
February (DJF) averaged sea surface temperature (SST) variability. Three such
teleconnections dominate. First, cool (warm) DJF SSTs in the equatorial Pacific Ocean
indicate the possibility (� � ≈ . ) of an early (late) AIRO date (Fig. 38). That is, La Niñas
(El Niños) often precede early (late) AIRO dates. Joseph et al. (1994) supports this claim,
noting that most significantly delayed onsets occur after an El Niño. Second, warm (cool) DJF
SSTs in the Mediterranean Sea significantly correspond (� � = − . ) to a subsequent early
(late) AIRO date (Fig. 38). While previous research has studied the relationship between
Mediterranean SST and Indian seasonal rainfall variability (Fontaine et al., 2011), no
research has analyzed the relationship between said SST and onset date variability
discovered herein. Finally, there is an oceanic phenomena located in the southern Pacific
Ocean called the South Pacific Dipole (SPD) (Guan et al., 2013). When DJF SSTs are cool
(warm) in the eastern SPD and warm (cool) in the western SPD, an early (late) AIRO date is
anticipated (� � = . ; Fig. 38). That is, a westward (eastward) DJF SST gradient across
35
the SPD suggests an early (late) AIRO date the following boreal spring or summer. These
DJF SST teleconnections can be monitored to provide a tentative estimate of the timing of
the following AIRO date.
The relationship of ENSO with ISM features may be analyzed in greater detail by
correlating monthly Niño 3.4 SSTs with AIRO, AIRD, total seasonal AIR, and June-
September (JJAS) All-India Monsoon Rainfall (AIMR, a commonly used index for
determining interannual ISM variability; Parthasarathy and Pant, 1985). The relationship
of Niño 3.4 SST with total seasonal AIR and AIMR is much more robust than its relationship
with AIRO and AIRD (Fig. 39). In fact, seasonal AIR and AIMR account for over 35% of the
variance in the subsequent ENSO mode (� ≈ − . ). Thus, a wet (dry) ISM offers greater
confidence that there will follow a La Niña (El Niño). ENSO and total monsoon rainfall are
linked by the westerly wind bursts over the tropical Pacific Ocean. Kirtman and Shukla
(2000) show that a weak (strong) monsoon leads to a weakening (strengthening) of the trade
winds, which in turn make a warm (cold) ENSO warmer (colder) approximately six months
later. Note also that the total seasonal AIR computed from the AIROD is very similar to the
JJAS AIMR, but it has higher values on average due to sampling before or after the JJAS
season (Fig. 40). Because the AIROD is intricately linked to large-scale phenomena which
influence the evolution of the ISM, total seasonal AIR’s flexibility likewise offers a more
physically-based depiction of the ISM than the static JJAS AIMR index does.
4.3.5 Moisture
Moisture-based variables also experience interannual variability in relationship with
the timing of the AIROD. Because vertically integrated moisture flux convergence is itself a
noisy variable as supplied by ERA-20C, its interannual variability is also quite complex. All
36
that can be confidently said about its relation to the AIRO is that there exists an increased
(decreased) anomaly of moisture convergence on the southwest Indian coast and in the upper
Bay of Bengal about fifteen days before and after an early (late) AIRO date, although the
exact location of this anomaly likely shifts significantly from year to year (Fig. 41). Even less
may be said concerning its interaction with the timing of the AIRD date (Fig. 42).
Precipitable water reveals a much clearer negative (positive) correlation (� � =− . ; � � = . ) with the AIRO (AIRD) date. There exists an anomalous increase
(decrease) in precipitable water compared to climatological values about ten days before an
early (late) AIRO date centered over the northeastern Arabian Sea, which then drifts over
north-central India by the AIRO and continues over the northern Bay of Bengal a few days
later. This excess (deficit) in precipitable water over north-central India during an early (late)
AIRO is balanced by a deficit (excess) in the surrounding domain (Fig. 43). Conversely, an
anomalous increase (decrease) in precipitable water over central India exists five days before
and after a late (early) AIRD date (Fig. 44).
This relationship between precipitable water and the AIROD is nearly replicated with
rainfall. By first observing the relationship between spatially-averaged AIR and the AIRO, a
significantly negative correlation is noticed from a little more than ten days before AIRO to
a little less than ten days after, with a minimum (� � = − . ) at AIRO (Fig. 45a). This
means that an anomalous increase (decrease) in AIR is associated with an anomalously early
(late) AIRO date. This is expected, for the AIROD is based upon AIR. Consequently, a positive
(� � = . ) correlation between AIR and the AIRD is observed roughly five days before to
just over ten days after the AIRD (Fig. 45b). Note that correlations become insignificant
outside of this range. Therefore, a portion of early and late seasonal rainfall variability may
be known if the AIROD variability is accurately predicted. The relationship between gridded
37
rainfall and the AIROD reveals that these negative (positive) anomalies, which are associated
with the AIRO (AIRD), occur predominantly over central India. Increased (decreased) rainfall
occurs in central India and along the central western coast prior to an early (late) AIRO date
and after a late (early) AIRD date (Figs. 46 and 47). While the location of anomalous rainfall
and precipitable water may be surprising considering that the greatest moisture exists over
Kerala and the seven sister states (Figs. 25-28), this result agrees with many previous studies
that have found central India to adequately represent variability across the entire Indian
subcontinent with respect to pressure, temperature, and rainfall anomalies (Hastenrath and
Rosen, 1983; Parthasarathy et al., 1990; Kumar et al., 1995). For this reason, anomalous
precipitable water and especially rainfall may be monitored prior to the AIRO to assist in
determination of its timing.
38
CHAPTER 5
CONCLUSION
The newly proposed All-India rainfall onset and demise (AIROD), an AIR-based index
that objectively determines the onset and demise dates of the Indian summer monsoon (ISM),
has been intricately examined. It is very simple, being based exclusively on rainfall averaged
over all of India, a variable which has been reliably observed for over a century and which
allows those outside of the scientific community to perceive ISM variability more easily.
Minimal resources would be required to supplement existing methods of monitoring the onset
of the ISM with the AIROD because of its very simple computation and its foundation upon
a rainfall dataset which is already monitored by the IMD. Furthermore, AIROD successfully
avoids all recorded false onsets and provides an onset date that closely parallels IMD onset
definitions.
The AIROD seems to be the most representative onset index proposed to date and is
intricately related to changes in large-scale phenomena that characterize the ISM. This index
is verified with the seasonal evolution of other dynamic (i.e. wind-based) and thermodynamic
(i.e. temperature- and moisture-based) variables of the ISM and is shown to be consistent
with their evolution. The zonal (meridional) progression of the reversal of the 300hPa
meridional temperature gradient (meridional ocean heat transport) may be detected almost
three weeks in advance of the onset, providing advanced warning of its timing. Moisture-
based features such as vertically integrated moisture flux convergence, precipitable water,
and rainfall are seen to dramatically increase (decrease) over Kerala and the seven sister
states prior to the onset (demise) and subsequently over central India. Wind-based features
such as 850hPa to 200hPa vertical wind shear and kinetic energy of the 850hPa winds also
increase rapidly over a few days off the Somali coast and extend eastward across the Arabian
39
Sea as the onset approaches. Similarly, 300hPa temperature is also seen to increase across
the domain, but most greatly over northeast India prior to onset.
Interannual variability of large-scale phenomena as a result of the timing of the
AIROD is also assessed. Total seasonal rainfall anomalies are captured by AIROD anomalies,
with early (late) onset and late (early) demise resulting in an increase (decrease) of seasonal
rainfall. This relationship indicates that close monitoring of the onset can provide additional
information about the development of an anomalous ISM season. In addition, seasonal
rainfall seems to be a good predictor of a subsequent ENSO mode, with a wet (dry) ISM
season preceding a La Niña (El Niño). Furthermore, the flexible nature of total seasonal AIR,
which is computed using the AIROD, offers a more accurate, physically-based depiction of
the interannual variability of the ISM than does the commonly-used JJAS All-India monsoon
rainfall (AIMR) index. DJF SST teleconnections also exist in relation to the timing of onset,
providing weak preliminary estimates almost half a year in advance. Two other potentially
useful indicators of the timing of onset are the zonal progression of the anomaly of kinetic
energy of 850hPa winds fifteen days prior, and the anomalous central Indian rainfall ten
days prior, to onset.
Research is currently underway to define local and regional transition dates that
would contribute to the currently-defined AIROD but offer a more useful application for end
users. The predictability of the AIROD using weather and climate models is also being
studied. ISM variability on longer than the interannual time scale will also be examined
using Empirical Ensemble Mode Decomposition (EEMD) analysis (Wu and Huang, 2009).
Other interesting future research may include application of the index to other variables with
strong seasonal cycles. One could determine annual onset dates each based on a different
large-scale variable, and then search for a consistent order of these dates. As each onset date
is triggered in a given year, forecasters would then be able to narrow their forecast for the
40
AIR-based onset date, which occurs last and represents the arrival of the ISM. Finally,
zonally-integrated meridional ocean heat transport must be investigated in greater detail
both to determine the cause of the order-of-magnitude discrepancy in this study and to better
understand the influence of boundary currents upon basin-wide transport.
41
APPENDIX A
TABLES
Source Variables Domain Large-scale transition
Rao (1976) Surface pressure and wind
Bay of Bengal:
north of 18N
Monsoon depressions (2-3 closed isobars at 2hPa
intervals over 5 square grid; surface winds 17-33kts)
Krishnamurti and Ramanathan (1982)
Zonal wind Arabian Sea:
50-70E, 4S-20N
850hPa kinetic energy of zonal wind increases by order of magnitude
Murakami and Nakazawa (1985)
Outgoing longwave radiation (OLR) and wind
Global Asymmetric component of OLR reverses and 200hPa velocity potential divergence transitions from Southern to Northern Hemisphere
Ananthakrishnan and Soman (1988)
Rainfall Kerala, India:
815’N-1250’N
Rainfall suddenly shifts from light (<10mmday-1) to strong (>10mmday-1) regime
Webster and Yang (1992)
Zonal wind 40-110E, 0-20N
850-200hPa vertical wind shear of zonal winds reverses
Yanai et al. (1992)
Temperature 40-130E, 0-50N
500-200hPa layer-mean meridional temperature
gradient from 5N to 25N reverses
Soman and Kumar (1993)
Rainfall, relative humidity (RH), vertically integrated zonal moisture transport (VIZMT), wind, and OLR
India (23 scattered stations)
Rainfall, RH, and VIZMT sharply increase, upper-tropospheric winds change strength and transition north, and OLR rapidly decreases
Table 1. Large-scale atmospheric and oceanic changes associated with onset from previous literature.
42
Source Variables Domain Large-scale transition
Lau et al. (1998)
Rainfall, precipitable water (PW), wind, and sea surface temperature (SST)
South China Sea
Rainfall transitions east and increases, PW increases, surface winds reverse, and Indian Ocean SSTs cool while subtropical western Pacific SSTs warm
Wu and Zhang (1998)
Sensible heat flux (SHF)
South and Southeast Asia
SHF maximizes over Tibetan Plateau and land-ocean contrast reverses
Goswami et al. (1999)
Meridional wind 70-110E, 10-30N
850-200hPa vertical wind shear of meridional winds reverses
Hsu et al. (1999)
Temperature, outgoing longwave radiation (OLR), zonal wind, diabatic heating, and SST
Southeast Asia Deep convection, diabatic heating, and North Indian Ocean SST suddenly increase and 200hPa and 850hPa zonal winds reverse, followed 850hPa cyclonic circulation developing and southwesterly wind strengthening
Loschnigg and Webster (2000)
Meridional current velocity and temperature
North Indian Ocean down to
20S
Meridional ocean heat transport reverses
Goswami and Gouda (2010)
Rainfall Kerala, India:
8-12N, 75-77E
Rainfall sharply increases
Table 1. Continued.
43
Source Variables Domain Onset Index
Ananthakrishnan et al. (1968)
Rainfall Kerala (seven stations)
- After 10 May, second in a period of two days when five of seven stations receive >1mm of rainfall
Ramage (1971) Wind Global - Prevailing wind direction shifts by at least 120 and persists for at least 40% of the time in January and July - Mean wind exceeds 3ms-1 in January or July - Fewer than one cyclone-anticyclone alternation occurs every two years in January or July in a 5 rectangle
Rao (1976) Rainfall Zonal wind Relative humidity
Kerala - Rainfall widespread with large amounts at individual stations which persists over several days - Lower-tropospheric westerlies strong and deep - High relative humidity up to at least 500hPa
Ananthakrishnan and Soman (1988)
Rainfall Kerala: 815’-1250’N
- First day with >10mm of rainfall in a period of five days with a daily average of >10mm
Fasullo and Webster (2003)
Vertically integrated moisture transport (VIMT)
Arabian Sea (50 largest vectors): 45-85E, 5-20N
- Day when normalized VIMT time series exceeds zero (i.e. Hydrological Onset and Withdrawal Index, or HOWI)
Janowiak and Xie (2003)
Rainfall Global - First in period of four pentads with rainfall for three out of four exceeding 33% of climatological rainy season mean rainfall
Zeng and Lu (2004)
Precipitable water
Global - First day when normalized precipitable water index (NPWI) is greater than the Golden Ratio (0.618) for three consecutive days in seven of nine 1°x1° cells
Prasad and Hayashi (2005)
Temperature Wind
40-80E, 10-17.5N 65-75E, 10-17.5N
- 850-600hPa zonal asymmetric temperature anomalies (ZATA) become negative for more than three days with a minimum of 10ms-1 of 850-200hPa vertical wind shear of zonal winds (VWSI)
Table 2. Onset indices from previous literature.
44
Source Variables Domain Onset Index
Taniguchi and Koike (2006)
Wind Arabian Sea: 62.5-75E, 7.5-20N
- First in period of seven days with wind speed continuously exceeding 8ms-1
Joseph et al. (2006)
Zonal wind Outgoing longwave radiation (OLR)
70-85E, 5-10N - Day when 6ms-1 mean zonal wind beginning at 850hPa crosses the 600hPa level, and passes bogus onset and widespread Kerala convection tests
Xavier et al. (2007)
Temperature Northern box: 40-100E, 5-35N Southern box: 40-100E, 15S-5N
- Difference in 600-200hPa averaged meridional temperature gradient between northern and southern boxes changes sign from negative to positive
Pai and Rajeevan (2009)
Rainfall Zonal wind OLR
14 Kerala stations 55-80E, 0-10N 70-75E, 5-10N
- After 10 May - Second of two consecutive days for which 60% of stations report 2.5mm - Zonal wind 15-20kts at 925hPa maintained up to 600hPa - OLR below 200Wm-2
Wang et al. (2009)
Zonal wind South Arabian Sea: 40-80E, 5-15N
- First in period of seven days with daily average 850hPa zonal wind exceeding 6.2ms-1
Goswami and Gouda (2010)
Rainfall Kerala: 75-77E, 8-12N
- First in period of three days with rainfall >3mm over 30% of domain region
Moron and Robertson (2014)
Rainfall India - First of 5 consecutive wet (10mm) days after 1 April that receives climatological 5 day wet spell amount in April-October without being followed by a 10 day dry spell (<5mm) in the following 30 days
Misra and DiNapoli (2014)
Rainfall Monsoon Asia: 60-150E, 0-55N
- Day when anomalous accumulation is above the annual mean
Table 2. Continued.
45
Source Dataset Variable Domain Grid
Spacing Temporal Resolution
Length
ATMOSPHERE IMD NCC
Gridded AIR Rainfall India 0.25 Daily 1902-2005
RIHN and MRI/JMA
APHRODITE Rainfall India and Bangladesh
0.25 Daily 1951-2005
ECMWF ERA-20C Precipitable water Vertically integrated moisture flux divergence Zonal and meridional wind velocity Temperature
50-110E, 0-40N 40-120E
0.25 Daily 1902-2005
OCEAN NCEP CFSR Potential
temperature Zonal and meridional current velocity
40-100E, 25S-25N
0.5 Daily 1979-2005
Met Office
HadISST1 Sea surface temperature
Global 1 Monthly 1902-2005
NCAR CGD CAS
N3.4 Niño 3.4 Index 120-170W, 5S-5N
N/A Monthly 1902-2005
Year False onset “Actual” onset AIRO 1946 12 May (Fieux and Stommel,
1977) 29 May (Ananthakrishnan and Soman, 1988)
4 June
1958 10 May (FS77) 14 June (AS88) 17 June 1967 17 May (FS77) 9 June (AS88) 11 June 1968 5 May (FS77) 8 June (AS88) 10 June 1972 16 May (NPTEL, 2013) 19 June (Pai and Rajeevan, 2009) 17 June 1979 9 May (Flatau et al., 2001) 12 June (PN09) 8 June 1986 10 May (F01) 12 June (PN09) 12 June 1995 9 May (F01) 10 June (PN09) 11 June 1997 14 May (F01) 12 June (PN09) 8 June 2002 29 May (Flatau et al., 2003) 9 June (PN09) 9 June 2004 18 May (SG) 3 June (PN09) 4 June
Table 3. Datasets implemented in this paper and their metadata.
Table 4. False o set years, a d their three perti e t dates: false o set, actual o set, a d AIRO.
46
Variable Parameters
Rainfall 1902-2005; 0.25 grid spacing; IMD-defined all-India domain
Precipitable water 1902-2005; 0.25 grid spacing; 50-110E and 0-40N Vertically integrated moisture flux convergence
1902-2005; 0.25 grid spacing; 50-110E and 0-40N
850hPa kinetic energy 1902-2005; 0.25 grid spacing; 50-110E and 0-40N 850-200hPa vertical wind shear
1902-2005; 0.25 grid spacing; 50-110E and 0-40N
300hPa temperature 1902-2005; 0.25 grid spacing; 50-110E and 0-40N 300hPa meridional temperature gradient
1902-2005; 0.25 grid spacing; 40-120E and 0-40N
Meridional ocean heat transport
1979-2005; 0.50 grid spacing; 40-100E and 25S-25N
Sea Surface Temperature 1902-2005; 1 grid spacing; global Niño 3.4 Index 1902-2005; 170-120E and 5S-5N
Table 5. Direct and derived large-scale atmospheric and oceanic variables analyzed in this study.
Table 6. Correlations between ISM features. Bolded values are significant at the 95% confidence interval.
47
Table 7. A ual total seaso al AIR, AIRO, AIRD, a d seaso le gth. These I“M features’ ea s a d sta dard deviatio s are
shown at the end of the table. All years with total seasonal AIR a standard deviation above (below) the mean are given in
blue (red) font.
49
APPENDIX B
FIGURES
Figure 1. Important locations referred to during this study.
Figure 2. The domains and rain gauge distributions used in APHRODITE V1101 for monsoon Asia (MA), the MIddle East
(ME), and northern Eurasia [i.e., Russia (RU)], and in V1005 for Japan (JP). Stations derived from the GTS network (blue
dots), those from the precompiled dataset (black dots , a d those i APHRODITE’s i dividual data collectio red dots . Taken from Yatagai et al. (2012).
50
Figure 3. Seasonal cycle of rainfall for the year 2000. Daily rainfall (orange) and cumulative anomalous rainfall (blue) are
depicted, and onset, peak, and demise dates are indicated by the black lines and corresponding dates.
Figure 4. The seasonal cycle of rainfall during the Maharashtra Drought of 1972. Daily rainfall (orange) and cumulative
anomalous rainfall (blue) are depicted. The red circle indicates day 1, which is the technical absolute maximum of
cumulative anomalous rainfall (as shown by the flat red line extending from its value). The red arrow indicates true demise
date, which becomes the absolute maximum of cumulative anomalous rainfall when applying the stipulation that demise
must occur after onset. While not shown above, dry years may also result in the absolute minimum occurring on the final
day of the year instead of occurring on the true onset date. This problem is alleviated by applying another stipulation that
the onset cannot occur during the last three months, or 92 days, of the year.
51
Figure 5. OLR in the middle of May for the four cases of multiple monsoon onset. OLR contours below 200 Wm-2, indicating
convection, are dark. Taken from Flatau et al. (2001).
52
d)
c)
a)
b)
Figure 6. AIR-based a) onset date, b) demise date, c) season length, and d) annual mean of AIR from 1902 to 2005. For a)-c),
the long-dashed black line is linear trend, and the short-dashed black line is the ten-year moving average. Note the
differences in values on the y-axes. d) Annual means of AIR (blue), with 5-, 15-, and 30-year moving averages (yellow, green,
and red dashed lines, respectively), linear trend (black dotted line), and standard deviation bars (light gray, deviating from
climatological annual mean for all 104 years) are plotted. No trend exists for the onset dates, and all trends are considered
insignificant according to Mann Kendall test.
53
Figure 7. Distribution of onset dates (top), demise dates (middle), and season length (bottom). Note that axis values are
different for each plot and that none are Gaussian.
54
Fig
ure
8.
Pa
ram
ete
rs c
ha
ract
eri
zin
g a
Ga
uss
ian
or
no
rma
l d
istr
ibu
tio
n.
Ta
ke
n f
rom
Bre
reto
n (
20
14
).
55
Figure 9. Brown shaded area represents the AIR region. The boxed region represents the Bangladesh region included in the
APHRODITE onset date test. The brown and boxed regions combined represent the APHRO domain. Image provided by
MapsOfWorld (2016).
56
Figure 10. Comparison of onset (top) and demise (bottom) dates for two spatially-averaged rainfall domains: AIR and
APHRO. The dotted lines are linear trends for their respectively colored time series.
57
Fig
ure
11
. S
ea
son
al
evo
luti
on
of
11
fa
lse
on
set
ye
ars
re
cord
ed
by
pre
vio
us
stu
die
s. T
he
ora
ng
e l
ine
s a
re t
he
da
ily A
IR,
the
ora
ng
e d
ash
ed
lin
es
are
th
e c
lim
ato
log
ica
l a
nn
ua
l
me
an
, a
nd
th
e b
lue
lin
es
are
th
e c
um
ula
tive
da
ily a
no
ma
ly o
f A
IR.
Th
e r
ed
ba
rs in
dic
ate
fa
lse
on
set,
th
e p
urp
le b
ars
in
dic
ate
ac
tual
ose
t as d
efi
ne
d b
y I
MD
, a
nd
th
e g
ree
n
ba
rs r
ep
rese
nt
AIR
O.
58
Figure 12. Ekman transport throughout the mixed layer (roughly 100m) of the ocean, where the competing Coriolis force
and turbulent drag slow and turn the direction of the current to the right at deeper depths. The longest arrow is the surface
current, which flows at a 45° angle to the right of the surface winds. Although not depicted, the averaged Ekman transport
flows perpendicular to the surface winds. Taken from Ekman (1905).
Figure 13. Simplified regulation of the seasonal cycle of the Indian Ocean in the boreal a) summer and b) winter, where
black arrows indicate the direction of near-surface winds and gray arrows indicated the direction of Ekman transport and
the resulting heat flux. Adapted from Loschnigg and Webster (2000).
59
Figure 14. Seasonal evolution of the daily composite (averaged over 104 years from 1902-2005) of 300hPa temperature
centered on the AIRO (time = 0) at intervals of five days. Units are in °K/1000km.
61
b)
a)
Fig
ure
16
. T
he
cli
ma
tolo
gic
al
da
ily z
on
al p
rog
ress
ion
of
the
me
rid
ion
al
tem
pe
ratu
re g
rad
ien
t b
etw
ee
n 5
°N a
nd
25
°N a
t 3
00
hP
a a
s a
fu
nct
ion
of
lea
d/l
ag
tim
e w
ith
re
spe
ct t
o
the
a)
AIR
O a
nd
b)
AIR
D f
rom
40
°E t
o 1
20
°E.
Un
its
are
in
°K
/10
00
km
. T
he
ze
ro c
on
tou
r li
ne
is
sho
wn
in
bla
ck.
63
Figure 18. Same as Fig. 14, but for 850hPa to 200hPa vertical wind shear centered on the AIRD. Units are in ms-1.
65
Figure 20. Same as Fig. 14, but for kinetic energy of 850hPa winds centered on the AIRD. Units are in m2s-2.
66
a) b)
Figure 21. The climatological daily meridional progression of zonally-averaged meridional ocean heat transport computed
to a depth of 105m (~mixed layer depth of the tropical Indian Ocean) as a function of lead/lag time with respect to the a)
AIRO and b) AIRD from 25°S to 25°N. Units are in 0.1PW. The zero contour line is shown in black.
Figure 22. Schematic of the horizontal velocity structure of the n=1 Rossby mode with southward Ekman flow added to
regions outside of the equatorial wave guide and cool colored pathways and streamlines indicating southward heat
transport. Warm colors indicate northward transport. Taken from Sahami (2003).
67
Figure 23. Same as Fig. 14, but for vertically integrated moisture flux convergence. Units are in 10-4kgs-1.
68
Figure 24. Same as Fig. 14, but for vertically integrated moisture flux convergence centered on the AIRD. Units in 10-4kgs-1.
73
a) b)
Figure 29. Correlation of a) AIRO and b) AIRD date anomalies with total seasonal rainfall anomalies. Only significant values
at 95% confidence interval are shown.
a) b)
Figure 30. Same as Fig. 29, but with 300hPa meridional temperature gradient from 5°N to 25°N at various lead/lag times
with respect to the a) AIRO and b) AIRD date.
74
Figure 31. Correlation of AIRO date anomalies with 300hPa temperature anomalies at various lead/lag times. Only
significant values at 95% confidence interval are shown.
77
Figure 34. Same as Fig. 31, but with 850hPa to 200hPa vertical wind shear anomalies and AIRD date anomalies.
79
Figure 36. Same as Fig. 31, but with kinetic energy anomalies of 850hPa wind and AIRD date anomalies.
80
a) b)
Figure 37. Same as Fig. 29, but with meridional ocean heat transport from 25°S to 25°N at various lead/lag times with
respect to the a) AIRO and b) AIRD date.
Figure 38. Correlation of AIRO date anomalies with global December-February averaged sea surface temperature
anomalies. Only significant values at 95% confidence interval are shown.
81
Fig
ure
39
. C
orr
ela
tio
n o
f m
on
thly
Niñ
o3
.4 s
ea
su
rfa
ce t
em
pe
ratu
re (
SST
) a
no
ma
lie
s w
ith
AIR
O d
ate
an
om
ali
es
(re
d c
ircl
es)
, A
IRD
da
te a
no
ma
lie
s (b
lack
sq
ua
res)
, to
tal
sea
son
al
AIR
an
om
ali
es
(blu
e c
ircl
es)
, a
nd
Ju
ne
-Se
pte
mb
er
(JJA
S)
AIR
an
om
ali
es
(gre
en
dia
mo
nd
s).
Th
e r
ed
an
d b
lack
arr
ow
s in
dic
ate
th
e c
lim
ato
log
ica
l A
IRO
an
d A
IRD
da
tes,
re
spe
ctiv
ely
. C
orr
ela
tio
ns
pri
or
to t
he
se d
ate
s w
ou
ld a
pp
roxi
ma
tely
co
rre
spo
nd
to
SS
T l
ea
din
g t
he
AIR
O/A
IRD
.
82
Fig
ure
40
. A
co
mp
ari
son
of
the
to
tal
sea
son
al
AIR
(b
lue
) a
nd
th
e J
un
e-S
ep
tem
be
r (J
JAS)
All
-In
dia
Mo
nso
on
Ra
infa
ll (
AIM
R;
ora
ng
e).
Th
e h
ori
zon
tal d
ash
ed
lin
es
wit
h
corr
esp
on
din
g c
olo
rs m
ark
on
e s
tan
da
rd d
evi
ati
on
be
low
an
d a
bo
ve t
he
ir r
esp
ect
ive
me
an
s.
84
Figure 42. Same as Fig. 31, but with vertically integrated moisture flux convergence anomalies and AIRD anomalies.
87
a)
b)
Figure 45. Same as Fig. 29, but with AIR anomalies at various lead/lag times with respect to the a) AIRO and b) AIRD date.
The composite daily rainfall (blue line; units in mm) is also plotted to show the sudden increase (decrease) at the AIRO
(AIRD). Correlation coefficient is plotted as the orange line, with missing values indicating insignificance at the 95%
confidence interval.
90
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BIOGRAPHICAL SKETCH
Education Florida State University, Tallahassee, Fl. – May 2016
M.S. Meteorology; Cum Laude; GPA: 3.88
Dean’s list (2014-2016) Thesis: Characterizing the onset and demise of the Indian summer monsoon
Virginia Tech, Blacksburg, Va. – May 2014 B.S. Meteorology, Magna Cum Laude; GPA: 3.65 Dean’s list (2010, 2012-2014)
Research Topics
Characteristics of onset and demise of the Indian summer monsoon
Precipitation characteristics in the visible, infrared, and microwave spectra Brownian motion
Aerosol-monsoon relationship
FSTRC radiation model analysis Atlantic warm pool influence on hurricane track
Latent heat contribution to Florida precipitation (Evaporation-precipitation feedback)
ENSO-East Pacific warm pool relationship
Atmospheric impacts on oceanic salinity variability
Scale analysis of observational parameterization on modeled flux variability Dual-Polarization winter precipitation detection
Professional Experience Florida State University, Tallahassee, Fl. ............................................................ 2015 to 2016
Meteorology Graduate Research Assistant [20hr/wk] Conducted research characterizing the onset and demise of the Indian summer monsoon to improve the lead time and accuracy of monsoon forecasting. Included professional collaboration, programming and plot production, critical thinking and analysis of unique data, and communication of novel results.
Florida State University, Tallahassee, Fl. ............................................................ 2014 to 2015 Meteorology Graduate Teaching Assistant [20hr/wk]
Assisted professor with educating and evaluating students by tutoring students on an individual need basis, leading classroom review in the professor’s absence, and grading/commenting homework.
Bus Transit, Blacksburg, Va. ................................................................................ 2012 to 2014 Bus Operator [13hr/wk] Transported passengers in a safe and timely manner, worked with 35 to 70 foot vehicles that require a Commercial Driver’s License (CDL).
Virginia Tech Writing Center, Blacksburg, Va. ................................................................. 2013 Writing Coach [5hr/wk] Guided students, including many ESL speakers, in improvement of their written communication and facilitated their linguistic competency; also corrected grammatical and syntactical errors.
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Leadership/Volunteer Experience Go2 Church, Tallahassee, Fl. ................................................................................ 2015 to 2016 Production/Vocalist team member
Oversaw light, sound, and media production in such a manner as to reduce distraction and facilitate an atmosphere of worship. Also led congregation in worship through song.
Earth, Ocean, and Atmospheric Sciences Thalassic Society, Tallahassee, Fl. .... 2015 to 2016 Treasurer [5hr/mo] Managed the organization’s funds to ensure fiscal responsibility, thus enabling current events and setting aside additional funds for future years.
Special Olympics Florida, Tallahassee, Fl. ........................................................................ 2015 Soccer unified partner/volunteer [3 weeks, 2.5hr/wk; for State Olympics, 15hr/day]
Assisted athletes in soccer practices and games as a player and mentor; also participated as a player, chaperone, and friend of athletes in the 2015 State Summer Special Olympics, where our team won a bronze medal.
Life Center Academy, Jaipur, Rajasthan, India ................................................................ 2013 Kindergarten teaching assistant [3 weeks, 30hr/wk] Primary objectives included teaching English numbers, letters, songs, and poems to impoverished Banjara children; enabling them to produce poems and songs of their own creative expression; and offering attention, care, and friendship rarely experienced outside of their school experience.
College of Natural Resources and Environment Leadership Institute, Blacksburg, Va. ...................................................................................................... 2012 to 2013
Cohort member [8hr/wk] Applied leadership principles to team projects; learned how leaders deal with change, teamwork, and conflict; leveraged personality types to work with and lead others; and networked with environmental leaders at state and national levels in both the private and public sectors.
Chi Alpha Christian Fellowship, Blacksburg, Va. ................................................ 2012 to 2013 International student leader [3hr/wk]
Facilitated relationship and communication between international students, encouraging conversation about significant life issues and cultural diversity.
Chi Alpha Christian Fellowship, Blacksburg, Va. ................................................ 2011 to 2012 Small group/ bible study leader [5hr/wk]
Other Experience National Weather Service, Blacksburg, Va. ...................................................................... 2014
Intern [10hr/wk] National Weather Service, Blacksburg, Va. ......................................................... 2013 to 2014
Researcher (Dual-Polarization Winter Precipitation Detection) [8hr/wk] Virginia Tech, Blacksburg, Va. .......................................................................................... 2013
Midwest storm chase member [12 days] Virginia Tech Writing Center, Blacksburg, Va. ................................................................. 2012
Writing center intern [5hr/wk] Virginia Tech, Blacksburg, Va. .......................................................................................... 2011
Intramural soccer team member [1hr/wk] Professional Organizations
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American Meteorological Society .......................................................................... 2015 to 2016 Chi Epsilon Pi Meteorology Honor Society ........................................................... 2015 to 2016 Earth, Ocean, and Atmospheric Sciences Thalassic Society ................................ 2015 to 2016 Computer Skills Programming languages
FORTRAN, GrADS (proficient) Matlab, shell scripting (elementary)
Operating systems Windows (excellent) Mac, Linux (proficient)
Other software Excel, PowerPoint, Word, Google Earth (excellent) ArcGIS, ESRI (elementary)
Language Experience Virginia Tech, Blacksburg, Va.
Ancient Greek [two semesters] Virginia Hummel Book Prize for Excellence in Ancient Greek (2014)
Life Center Academy, Jaipur, Rajasthan, India Hindi [three weeks]
Travelled to India Warhill High School, Williamsburg, Va.
Spanish [four years] Travelled to Costa Rica and Honduras [two and a half weeks]