IAPRS & SIS, Vol.34, Part 7, "Resource and Environmental Monitoring", Hyderabad, India,2002
2.1 Approach
A physical retrieval scheme (Appendix I) developed by
Tanahashi et al. (2001) for deriving surface insolation on
operational basis from VISSR-GMS-5 in Japan is adopted to
Meteosat data for present study. The different steps are given
below.
1).Cloud detection and characterization was found out by
bispectral threshold technique using visible and thermal band
data from a time series of images of 30 days in December 1998.
2) Latitude and longitudes corresponding to METEOSAT lines
and pixels were generated using algorithm given by
EUMETSAT.
3) Solar Zenith angle 0) layer was generated from latitude,
. longitude, Julian day of the year and time of the day.
4) Atmospheric correction was carried out with respect to
atmospheric costitituents such as: ozone, water vapor, aerosol
which are contributing to atmospheric turbidity.
5) The daily total surface insolation was computed by Simpson
integration of hourly insolation at five different times in a day.
The inputs to this model are listed below:
i) A time series of images of visible, thermal IR bands for
particular acquisition time
ii) Day of the year and time in a day
iii) Solar zenith angle
iv) Cloud attenuation coefficients for different cloud classes
V) Average ozone content
vi) Total atmospheric precipitable water
vii) Average Angstrom turbidity parameters to determine
aerosol transmittance in a season
The surface insolation (Sg) is derived by the following
equation.
Ss = (Sı+Sp+Sa)(1-2.A) <<)
Where, cloud attenuation coefficients (a) to insolation were
derived from look-up table of cloud top albedo (A) and
brightness temperature (TBB) given by (Tanahashi et al., 2001).
Direct (S;) and diffuse irradiation components due to Rayleigh
(Sg) and aerosol (SA) scattering were found out.
Se=S;tSptSa tone BUS Sy. 0 0 n. or. ror 77 (2)
SESTO OT dn A er où CT (3)
SE = ST (0. TR 1 5; 1t: vp ae vui (4)
S. zSlolmi-a.Eowa(- TA). fon nali mad L^ (5)
S-Lecos0 |... :,, , —, T . -— (6)
Where, S is the total surface insolation.
e = correction for sun-earth distance , which is 0.9674 on July 5
and 1.0344 on January 3.
Io7solar constant (1367 Wm?)
Transmittance due to absorption (To) by ozone was estimated
by the following equation
To71-0.02118(um)/(1--0.042(um)43.23x10 *(um)?)-1.082u/
(1+138.6(um))°*°*- 0.0658(um)/(1+(103.6(um))) ^ — -— (7)
Where, m is air mass= 1/ (cos0+0.15(93.885-6)"!2**)
u = Ozone content in atm-cm.The mean value of ozone is 0.3
atm-cm during December over india
Transmittance due to Rayleigh (Tg ) scattering was computed
as function of central wavelength of visible band.
Transmittance due to attenuation by aerosols(TA ) was
estimated by the equation below.
T,=0.10445a-0.0162+(1.003-0.125)xexp(-Bm(1.0890
505123) 0° fémote sensing, China, 15-2! Noveraa: (8)
a,=2.9wm/((1+141.5wm)0.635 + 5.925 wm) | . -—— (9)
where a, « and p are water vapor absorption coefficient and
Angstrom's turbidity parameters. Values are available from
Iqbal's table (Iqbal, 1983)
tw *' is precipitable water in cm. The NOAA TOVS (Tiros
operational vertical sounder) derived total precipitable water
(19x19) was used under present study.
3. RESULTS AND DISCUSSION
3.1 Sensitivity analysis
Since the different atmospheric parameters play major role to
influence the absorption and scattering processes of shortwave
incoming radiation, the sensitivity of surface insolation output
and direct to diffuse insolation ratio to a given change within
theoretical ranges of total precipitable water (w), angstrom
turbidity parameters for aerosol transmittance,o and p, was
studied. The results are presented in figures 1a,1b and 1c.
Sensitivity : atmospheric precipitable water (w)
1000
(a)
w=0.0
15
SE 900 | e
z €
g =0.5 2
$ ais 3
© me EST Po aime FFT 1Œ
$ =
z ren CICR E
© 800 4 a
E
w=0.0,0.5,1.0,2.0,3.0 L5
total insolation
* * * ? direct/diffuse
700 0
330 335 340 345 350 355 360 365 370
Julian day
Fig 1. (a) Sensitivity analysis of insolation retrieval scheme to
different atmospheric inputs
au eus. a 43 A SEAT SEA
TI
pr
ur
ab
de
tu
re
be
re
de
CO
in
Fc
av
D
or
hc