26
Variations in CERES- Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA- LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

  • View
    219

  • Download
    0

Embed Size (px)

Citation preview

Page 1: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Variations in CERES-Terra Fluxes and Cloud Properties with

SST Anomalies

Zach Eitzen (SSAI/NASA-LaRC)

Kuan-Man Xu (NASA-LaRC)

Takmeng Wong (NASA-LaRC)

Page 2: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Acknowledgments

• Thanks to David Doelling and Michele Nordeen for help with CERES cloud property data.

Page 3: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Motivation

• Recent authors (e.g., Wagner et al. (2008, Atmos Chem Phys) have used satellite data to examine cloud properties and their changes with SST anomaly.

• Others (e.g., Bony et al. 2004, Klein and Hartmann 1993, Wood and Bretherton 2006) have studied how clouds change with dynamical regime and lower-tropospheric stability.

• Here, we look at changes in cloud properties with SST anomaly, and attempt to quantify the portion of that change that is due to shifts in stability within a given dynamical regime.

Page 4: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Data Sources• All data is from March 2000-Feb 2005.• Monthly mean 1x1 degree CERES-EBAF data is used

for radiative fluxes.• Monthly mean 1x1 degree CERES Terra SRBAVG Non-

GEO data is used for optical depth and cloud fraction and cloud top height.

• Monthly mean Reynolds SSTs from NOAA.• ECMWF-Interim data is used for meteorological data,

including 700 and Estimated Inversion Strength (EIS).• “Standard” anomalies are calculated by subtracting each

month’s value from the five-year mean for that month. • Residual anomalies of cloud and radiative properties are

calculated by taking the mean anomaly associated with a given (700, EIS) state and subtracting it from the standard anomaly.

Page 5: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Change in total cloud fraction with SST (%/K)

Page 6: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Change in ln(tau) with SST (K-1)

Page 7: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Change in LW CRE with SST (W m-2 K-1)

Page 8: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Change in SW CRE with SST (W m-2 K-1)

Page 9: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Change in Net CRE with SST (W m-2 K-1)

Page 10: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Low cloud regions from Jensen et al. (2008)

Page 11: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Frequency of EIS-700 regimes

Page 12: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Average low cloud anomalies

Page 13: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Joint distribution of low cloud fraction and SST anomalies

Page 14: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Average low cloud ln() anomalies

Page 15: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Average SW CRE anomalies

Page 16: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Average Net CRE anomalies

Page 17: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Changes in properties with SST

Property Slope with standard anomalies

Slope with residual anomalies

Low Cloud Fraction -4.4 % K-1 -1.8 % K-1

Low Cloud ln() -0.103 K-1 -0.049 K-1

LW CRE 1.3 W m-2 K-1 0.5 W m-2 K-1

SW CRE 3.4 W m-2 K-1 2.1 W m-2 K-1

Net CRE 4.7 W m-2 K-1 2.6 W m-2 K-1

Page 18: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Summary• Near the ITCZ, cloud top heights, cloud fraction

and cloud optical depth all increase with SST, leading to little change in net CRE.

• In subtropical boundary-layer cloud regions, cloud fraction and cloud optical depth decrease with SST, leading to less shortwave cooling.

• Changes in cloud and radiative properties with SST have a strong association with changes in EIS within each dynamical regime, but there appears to be a positive cloud feedback even after this is removed.

Page 19: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Future Work• Look at additional fields.

• Filter out months with too much high cloud occurrence.

• Look at individual regions.

Page 20: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Change in cloud top height with SST (km/K)

Page 21: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Frequency of EIS-700 regimes

Page 22: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Average LW CRE anomalies

Page 23: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Joint distribution of low cloud ln() and SST anomalies

Page 24: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Joint distribution of SW CRE and SST anomalies

Page 25: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Joint distribution of LW CRE and SST anomalies

Page 26: Variations in CERES-Terra Fluxes and Cloud Properties with SST Anomalies Zach Eitzen (SSAI/NASA-LaRC) Kuan-Man Xu (NASA-LaRC) Takmeng Wong (NASA-LaRC)

Joint distribution of Net CRE and SST anomalies