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Journal of Basic and Applied Sciences Vol. 5, No. 2, 73-77, 2009 ISSN: 1814-8085
ESTIMATION OF GLOBAL AND DIFFUSE SOLAR RADIATION
FOR HYDERABAD, SINDH, PAKISTAN
M. Akhlaque Ahmed, Firoz Ahmad
1 and M. Wasim Akhtar
2
Basic and Applied Science, Sir Syed University of Engineering and Technology, Karachi, Pakistan 1Energy and Environment Research Group, Department of Physics, University of Karachi, Karachi, Pakistan
2Usman Institute of Technology, Karachi, Pakistan
ABSTRACT
Solar radiation studies have been carried out to asses the feasibility of solar Energy utilization at Hyderabad, Sindh,
Pakistan(Latitude25° 35′ N). The result obtained shows the variation of Direct and Diffuse component of solar radiation
in summer and winter months. The contribution of diffuse solar radiation is high during the monsoon months (July and
August) whereas sky condition are clear during winter months. From the estimated values it is found that with the
exception of monsoon month, solar energy can be utilized very efficiently throughout the year.
Keywords: Direct and Diffuse radiation, Sky Condition, Clearness Index, Hyderabad Sindh Pakistan.
INTRODUCTION
With the rapid depletion of fossil fuel reserves, it is feared
that the world will soon run out of its energy resources.
This is a matter of concern for the developing countries
whose economy heavily leans on its use of energy. Under
the circumanstances it is highly desirable that alternate
energy resources should be utilized with maximum
conversion efficiency to cope with the ever increasing
energy demand. Among the non-conventional energy
resources, solar energy, wind energy and Biomas has
emerged as most prospective option for the future.
Detailed information about the availability of solar
radiation on horizontal surface is essential for the
optimum design and study of solar energy conversion
system. For a country like Pakistan, the economical and
efficient application of solar energy seems inevitable
because of abundant sunshine available throughout the
year. Solar radiation data are available for most part of the
world, but is not available for many countries which can
not afford the measurement equipment and techniques
involved. Global solar radiation in Pakistan are measured
at five stations namely Karachi, Lahore, Multan, Quetta
and Islamabad, while diffuse solar radiation are not
observed experimentally in any Meteorological station of
the country. Therefore, it is rather important to develop
method to estimate the global and diffuse solar radiation
using climatological parameters. Several empirical
formula have been developed to calculate the global solar
radiation using various parameters. These parameters
includes i) The sunshine hours (Angstrom, A 1924,
Black, T.N et al., 1954,Glove et al., 1958) ii) The relative
humidity and sunshine hours (Gopi Nathan 1988), the
declination angle and the latitude(Liu, H et al., 1960), The
no of rainy days , sunshine hours latitude and
locations(Ready, 1977), sunshine duration, Relative
humidity max. temperature, latitude, altitude and
location(Sabbagh et al. 1977) and the total ppt, water,
turbidity and surface albedo(Hoyt 1978).
Besides this many other workers have reported the
estimation of Global and Diffuse solar radiation
employing various climatological parameters (Abdullah et
al., 1988, Chandal et al., 2005,Ahmad et al., 2004, Udo
2002, Togrul 2002).
In the present work, solar radiation estimation have been
done for the first time for Hyderabad Sindh, to utilize
solar energy for useful purpose. Prior to this work,
estimation of wind energy potential has also been reported
(Ahmad et al., 2004).
The Hyderabad city has an area of 5519 sq.Km. It is
located at latitude (Φ=25.35° N) and longitude 68o16
/.
east. It is the second largest city of Sindh province having
a population of 2.9 million people. About 50 percent of
this population lives in villages.
The city is famous for its “Wind Catch Chimmnies” over
the houses for intercepting wind, since old days. This
work will help the energy strategist and planners to utilize
the wind and solar energy potential to solve the energy
deficit in this city of abundant sunshine and strong wind,
throughout the year.
METHODS OF PREDICTION
Among the above mentioned empirical models, the most
popular is the regression equation of the Angstrom type
[1].
H/H0 = a + b ( n/N) (1)
Where H is the monthly average daily global solar
radiation falling on a horizontal surface at a particular
J. basic appl. sci.
74
location. Ho is the monthly mean daily radiation on a
horizontal surface in the absence of atmosphere. n is the
monthly mean daily number of hour of observed sunshine
hours , N is the monthly mean value of day length at a
particular location. a and b are climatologically
determined regression constant. n/N is often called the
percentage of possible sunshine hour.
Regression coefficient ”a” and “b” have been obtained
from the relationship given as(Tiwari & Sangeeta 1977)
and also confirmed by Frere et al. method[Frere et
al.1980].
a=-0.110+0.235 cos Φ+0.323(n/N)
b=1.449-0.553 cos Φ-0.694 (n/N) (2)
whereas there are many methods to evaluate these
constants (Ulfat et al., 2005).
For equation (1) the value of H0 is determined using
equation (1.8.3) of Duffi and Beckman (Duffie &
Backman 1991).
Ho = 24/ π Isc ( [1+0.033cos (360n/365)][ cosΦ cosδ sinws
+2Π ws /360sinΦ sinδ] (3)
Where Isc is the solar constant, Φ is the latitude, δ is the
solar declination, ws is the sunset hour angles where
δ =23.45 sin{360*248+n/365} (4)
and { cosws= -tanΦ tanδ } (5)
Prediction of Diffuse Solar Rdiation.Hd
The diffuse solar radiation Hd can be estimated by an
empirical formula which correlates the diffuse solar
radiation component Hd to the daily total radiation H. The
correlation equation which is widely used is developed by
Page (Page, Jk 1964).
Hd /H= 1.00-1.13KT (6)
Where Hd is the monthly mean of the daily Diffuse solar
radiation and KT =H/H0 is the clearness index. Another
commonly used correlation is due to Liu and Jordan
(1960) and developed by Klein (Klein SA, 1977) and is of
the form
Hd /H = 1.390-4.027 KT +5.53 ( KT )2 -3.108 ( KT )
3 (7)
RESULTS AND DISCUSSION
The input parameter for the estimation of monthly
average daily global solar radiation at Hyderabad, Sindh,
Pakistan are shown in Table 1. From this it is observed
that sunshine duration is above 70 percent throughout the
year; with the exception of July-August. Employing these
parameters the regression constant “a” and “b” are
evaluated as a=0.323 and b=0.470. Inserting these values
in equation (1) the monthly average daily Global solar
radiation H is estimated (Fig. 1). The value of H, KT, and
Hd for Hyderabad obtained through various correlation are
shown in Table 2. Also shown in this table is the ratio
D/H0 which shows that for Hyderabad the fraction of
diffuse radiation to Extraterrestrial radiation is not more
than 15 percent, with the exception of July-August.
Diffuse Solar Radiation
The diffuse solar radiation for Hyderabad is estimated by
Page and Liu and Jorden method, as no station in Pakistan
measures Diffuse solar radiation. From the estimated
results it is seen that contribution of diffuse solar radiation
is very low throughout the year with the exception of
monsoon months. The Liu and Jordan method predicts
lower values than the Page correlation. In the absence of
measured values of diffuse radiation it is difficult to
establish the superiority of one over the other. The
contribution of diffuse radiation is below 25 percent.
The availability of direct radiation is therefore very
encouraging from utilization point of view. The
transmission of Hd in Extrateresterial radiation is only 16
percent which rises to 20 percent in July-August. From
the observation of clearness index and ratio of diffuse to
global we conclude that presence of clouds is very rare
even in the monsoon months. This is the most favourable
condition for solar energy utilization.
Fig. 1 presents the plot of global solar radiation at
Hyderabad along with the sunshine Hour and the diffuse
solar radiation estimated by Liu and Jorden and Page
method. A dip is seen for the months of August for
n(Sunshine hour) and hence in the value of H, the global
solar radiation.
Fig: 1 Monthly variation of H,n.Hd (Page and LJ method) for
Hyderabad Sindh.
0
5
10
15
20
25
30
Jan
Feb
Mar
chApr
il
May
June
July
Aug
u.
Sep
t.Oct
Nov.
Dec.
Months
H m
jmd
H
n
Hd Page
Hd LJ
Fig. 1. Monthly variation of H,n,Hd (Page and Liu and
Jorden method) for Hyderabad, Sindh, Pakistan.
Ahmed et al.
75
The transmission through the atmosphere KT alongwith
the percent of diffuse radiation in global radiation is
shown in Fig. 2. The dip in the value of KT is in
accordance with the high value of Hd /H for the same
month. The sky is fairly clear during winter months when
solar radiation is in demand for utilization purpose.
Fig:2 Plot of Monthly variation of clearness index KT Hd/H
Page,Hd/H for LJ and Hd/H0 for Hyderabad, Sindh.
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
Jan
Feb
Marc
h
April
May
Jun
July
Aug.
Sept.
Oct
Nov.
Dec.
Months
Ratios
Kt
Hd/Hpage
Hd/H LJ
D/H
Fig. 2. Plot of Monthly variation of clearness index KT ,
Hd /H, (Page and LJ) and Hd /H0 for Hyderabad Sindh,
Pakistan.
Sky Condition: Hyderabad
The transparency of the atmosphere is indicated by
fraction of Extraterrestrial radiation that reaches the earth
surface as global solar radiation. It is a measure of the
degree of clearness of the sky. Clearness index is given as
KT =H/ H0
Where KT is clearness index, H is the global solar
radiation and H0 is the Extraterrestrial insolation.
From the estimated value of H for Hyderabad, KT is
calculated and it is very encouraging to note that the sky
over Hyderabad is very clear almost throughout the year
with exception of Jul-Aug. where KT <0.50 (i.e 50
percent).
Statistical Distribution Shown below is the statistical distribution of global solar
radiation which indicates that the availability of global
solar radiation at Hyderabad is well above 70 percent
during summer and winter months while it is only 50
percent in months of July-August which is the monsoon
period in this region.
Statistical Data of Global Solar Radiation
Jan-April Above 67 percent
May-Jun Above 60 percent
Jul-Aug (Monsoon) Above 50 percent
Sept-December Above 65 percent
Variation of Direct and Diffuse Solar Radiation:
Monthly Variation
A large variation in the intensities of Direct and Diffuse
radiation due to cloudiness have been indicated as stated
earlier. The result of the variation is plotted in Fig. 3 to
exhibit the trend of percentage variation of direct and
diffuse solar radiation. The maxima of direct radiation for
the month of April and Nov. are quite appreciable. The
percentage of diffuse radiation contributing to global
radiation is low during winter months (bright clear sky)
and does not exceed 40 percent even in the worst sky
condition. This is confirmed with the low values of KT
and high values of Hd /H (Fig. 2). The result obtained for
Hyderabad Sindh is in accordance with the results of the
earlier work done for Karachi, Pakistan (Ahmad
et.al.1981). The presence of direct radiation in April and
Nov. will be very useful for utilizing it for solar
concentrators, solar cookers and solar furnaces etc. The
Angstrom model for determination of Global solar
radiation and Liu and Jorden model for the estimation of
Diffuse solar radiation exhibits the validity of estimation
for the location under study.
Fig:3 Percentage variation of Direct and Diffuse radiation at
Hyderabad, Sindh,Pakistan.
0
10
20
30
40
50
60
70
80
90
Ja
n
Fe
b
Ma
rch
Ap
ril
Ma
y
Ju
ne
Ju
ly
Au
gu
.
Se
pt.
Oct
No
v.
De
c.
Months
Pe
rce
nta
ge
of
rad
iatio
n.
Direct
Diffuse
Fig. 3. Percentage variation of Direct and Diffuse
radiation at Hyderabad, Sindh, Pakistan.
CONCLUSION
The work reported in this paper indicates that the solar
energy utilization has bright prospects in Hyderabad.
Sindh, Pakistan. The estimated values of global and
J. basic appl. sci.
76
diffuse radiation reveals that solar radiation can be very
efficiently used to compensate for the energy deficit. For
the estimation of diffuse radiation Page and Liu and
Jordan methods are in very good agreement whereas
Angstrom equation calculates the monthly average daily
global solar radiation. Since no research regarding the
potential of solar energy has been done prior to this work,
this work will be very helpful to use these resources at
Hyderabad Sindh. Since the experimental data of Global
and diffuse solar radiation is not available for Hyderabad,
Sindh, the estimation has to be done employing sunshine
hours of the location. Linear and quadratics regression
could be developed, if the measured data for the location
under study is available. However the present work
employing Angstrom-model and Page and Liue and
Jorden model for Global and diffuse solar radiation for
Hyderabad Sindh, serves the purpose very effectively.
The wind energy potential is also encouraging as stated
earlier. Therefore a combination of solar and wind energy
availability will be very helpful in future to use this
tremendous amount of sunshine and high wind energy
potential.
REFERENCES
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Table 1. Input Parameters for Estimation of Monthly Average Global Solar Radiation at Hyderabad, Sindh, Pakistan
Months n
(Monthly mean sunshine Hour)
N
(Monthly Average Day length)
n/N(Percentage of
possible sunshine hour)
Jan 7.7 10.62 o.725
Feb 8.7 11.16 0.779
Mar 8.89 11.85 0.750
Apr 9.95 12.61 0.789
May 9.06 13.24 0.684
June 8.41 13.54 0.621
July 7.07 13.41 0.527
Aug 4.77 9.17 0.520
Sep 7.72 12.14 0.636
Oct 8.69 11.40 0.763
Nov 8.89 10.76 0.826
Dec 7.96 10.46 0.761
Table 2. Solar Radiation Data for Hyderabad, Sindh, Pakistan
Months Hest
MJm2d
Ho
MJm2d
- KT=H/H0
Hd / H
Page
Hd / H
LJ
Hd
Page
MJm2d
Hd
LJ
MJm2d
-
Hd /H0
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Apr 25.68 37.01 0.693 0.216 0.222 5.54 5.70 0.151
May 25.34 39.32 0.644 0.272 0.256 6.89 6.48 0.169
June 24.62 40.04 0.604 0.307 0.246 7.66 6.05 0.169
July 22.56 39.53 0.570 0.355 0.318 8.00 7.17 0.191
Aug 18.75 37.70 0.497 0.438 0.377 8.21 7.00 0.201
Sep 21.24 34.16 0.621 0.298 0.277 6.33 5.88 0.178
Oct 19.96 29.28 0.681 0.230 0.228 4.59 4.55 0.156
Nov 17.93 24.63 0.727 0.192 0.196 3.38 3.45 0.127
Dec 15.30 22.49 0.680 0.231 0.238 3.53 3.64 0.159
Ahmed et al.
77
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