GLI-weighted solar irradiance table

GLI NASDA Calibration Team, (minor calculation error was fixed on 24 March 2003)
PDF file

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.

GLI._WEIGHTED_IRR_EQ.JPG

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.

Calibration HomeGLI HomeEORC Home