GLI-weighted solar irradiance table
GLI NASDA Calibration Team,
(minor calculation error was fixed on 24 March 2003)
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We calculated GLI-band solar irradiances that have been weight-integrated the Thuillier-2002 solar spectral irradiance by spectral responses of every GLI bands. The GLI spectral response is running averaged +/-2 samples (data interval is about 1nm) window to reduce a measurement noise, and both response and solar irradiance datasets are linearly interpolated to 0.1nm spectral resolution before the integration. The weighted integration is operated as follow.
F0 is the GLI-weighted solar irradiance, E0 the Thuillier-2002 solar spectral irradiance, Rb, GLI spectral response for band b, N1 and N2 are minimum and maximum wavelength where both the GLI response and Thuillier-2002 solar irradiance are available. From channel 30 (3.7um) to 36 (12um) where Thuillier 2002 cannot cover, we used MODTRAN 4.0 for the calculation.
The calculated F0 are shown in Table 1. GLI calibration group will use the following F0 (*1). However, another F0 (*2) integrated within +/-2Dl (Dl is width of half peak power) are used when the precision is enough for the analysis target.
Table 1: Calculated channel-weighted solar irradiance values for all GLI channels
GLI channel |
F0 [W m-2um-1]
*1 |
F0 [W m-2um-1] +/-2Dl*2 |
source |
1 |
1095.696 |
1095.088 |
Thuillier
2002 |
2 |
1540.339 |
1540.261 | |
3 |
1714.570 |
1714.271 | |
4 |
1885.797 |
1885.786 | |
5 |
2082.035 |
2082.209 | |
6 |
1939.790 |
1939.741 | |
7 |
1792.522 |
1792.354 | |
8 |
1858.035 |
1858.094 | |
9 |
1788.986 |
1788.717 | |
10 |
1651.198 |
1651.271 |
Thuillier 2002 |
11 |
1522.468 |
1522.999 | |
12 |
1474.721 |
1474.566 | |
13 |
1479.008 |
1478.794 | |
14 |
1394.024 |
1393.808 | |
15 |
1396.239 |
1396.006 | |
16 |
1274.120 |
1274.033 | |
17 |
1248.869 |
1248.857 | |
18 |
956.023 |
956.079 | |
19 |
956.757 |
957.039 | |
20 |
1965.331 |
1965.345 |
Thuillier 2002 |
21 |
1838.794 |
1838.836 | |
22 |
1532.625 |
1532.605 | |
23 |
1061.675 |
1061.651 | |
24 |
654.572 |
654.581 |
Thuillier
2002 |
25 |
547.602 |
547.606 | |
26 |
454.842 |
454.750 | |
27 |
363.501 |
363.498 | |
28 |
233.004 |
233.004 |
Thuillier 2002 |
29 |
86.684 |
86.684 | |
30 |
11.596 |
11.576 |
MODTRAN4.0 |
31 |
1.164 |
1.164 | |
32 |
0.835 |
0.835 | |
33 |
0.760 |
0.759 | |
34 |
0.441 |
0.440 | |
35 |
0.185 |
0.185 | |
36 |
0.121 |
0.120 |
Reference
Thuillier, G., M. Hers, P. C. Simon, D. Labs,
H. Mandel, D. Gillotay, and T. Foujols, The solar spectral irradiance from 200
to 2400 nm as measured by the SOLSPEC spectrometer from the ATLAS 1-2-3 and
EURECA missions, Solar Physics, to be submitted, 2002.
Berk, A., and
co-authors, 1999: MODTRAN4 radiative transfer modeling for atmospheric
correction, SPIE proceeding, Optical Spectrocopic, Techniques and
Instrumentation for Atmospheric and Space Research III, Volume
3756.