The Relationship Between Incoming Solar Radiation and Daily Air Temperature
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University of Ghana
Abstract
Solar radiation is the ultimate source of energy for the planet. To predict the values of temperature
and instant solar radiation when equipment are not readily available from obtained equations, a
good knowledge and understanding of the disposition and distribution of solar radiation is a
requirement for modelling earth’s weather and climate change variables. A pyranometer (CM3) in
series with a PHYWE amplifier and a voltmeter were experimentally set-up and used to study the
amount of solar radiation received at the Physics Department of the University of Ghana during
the day. The temperature of the study area as well as the Relative Humidity was also recorded.
Data was collected over a period of one month (from 2 nd to 24 th April, 2012). Days for which rain
was recorded were ignored because rain could damage the pyranometer. The data obtained by the
set-up were therefore used to compare with data obtained by a wireless weather station (Davis
Vintage Pro). The data from these separate set-ups indicated that a perfect correlation existed
between the solar radiation and temperature of the place. The data obtained by the experimental
set-up was split into two separate sessions as morning and evening sessions. It was observed that
the experimental set-up had a good correlation with that of the weather station on a particular day
11 th April, 2012. The various Regression Coefficient (R 2 ) values for morning session were
respectively R 2 = 0.96 and R 2 = 0.95 with their respective equations as I W = 136.22T W −
40623 and I p = 2.3198T P − 678.14. The evening session also had good Regression Coefficient
values of R 2 = 0.81 and R 2 = 0.97 with equations of I P = 2.1098T P − 625 and I W =
161.31T W − 48769. Similar analysis of the data from the separate set-ups gave a better correlation
for that of the experimental set-up than that of the wireless station. The range of values of
Regression Coefficient (R 2 ) for the experimental set-up was between 0.82 − 0.99 for the morning
and 0.45 − 0.98 for the evening while the wireless station had 0.10 − 0.95 for the morning and 0.18 − 0.98 for the evening sessions. Analysis performed on the data set for the entire period
indicated that a strong correlation existed between the mean solar radiation (I m ) and the mean
temperature (T m ). The equations obtained for both set-ups for the morning and evening sessions
were found to be; I m = 2.417T m − 713 with a Regression Coefficient (R 2 ) value of 0.98 and
I m = 3.265T m − 974 with a Regression Coefficient (R 2 ) value of 0.97.
Description
Thesis (MPhil)-University of Ghana, 2013
