Operational Calibration of the Imagers and Sounders
|
| Channel | Nominal center wavenumber (cm-1) | # of detectors in N-S array | Detector FOV (km) | Detector material |
|---|---|---|---|---|
| 1 | 16000 (visible) | 8 | 1 | Si |
| 2 | 2555 | 2 | 4 | InSb |
| 3 | 1480 | 1 | 8 | HgCdTe |
| 4 | 935 | 2 | 4 | HgCdTe |
| 5 | 835 | 2 | 4 | HgCdTe |
| Channel | Nominal center wavenumber (cm-1) | Detector material | Channel | Nominal center wavenumber (cm-1) | Detector material |
|---|---|---|---|---|---|
| 1 | 680 | HgCdTe | 10 | 1345 | HgCdTe |
| 2 | 696 | HgCdTe | 11 | 1425 | HgCdTe |
| 3 | 711 | HgCdTe | 12 | 1535 | HgCdTe |
| 4 | 733 | HgCdTe | 13 | 2188 | InSb |
| 5 | 748 | HgCdTe | 14 | 2210 | InSb |
| 6 | 790 | HgCdTe | 15 | 2245 | InSb |
| 7 | 832 | HgCdTe | 16 | 2420 | InSb |
| 8 | 907 | HgCdTe | 17 | 2513 | InSb |
| 9 | 1030 | HgCdTe | 18 | 2671 | InSb |
| 19 | 14367(visible) | Si |
The spectral intervals in the infrared are isolated by a rotating wheel of filters. The filters are placed on the wheel in three concentric circles, which correspond to the channels of the three wavenumber regions--longwave (channels 1-7), midwave (channels 8-12), and shortwave (channels 13-18). Adichroic beamsplitter and a fixed filter isolate the visible channel. There is a north-south array of four detectors for each of the three infrared wavenumber regions, and a similar four-detector array for the visible. Each detector has a field of view (FOV) of approximately 8 km. Imager outputs are transmitted to the ground station as 10-bit words, sounder outputs as 13-bit words.
Before the launch of each satellite, the radiometric performance of the instruments was characterized in an extensive program of pre-launch tests conducted by their manufacturer (ITT, Ft. Wayne, IN) and by the GOES I-M prime contractor (Space Systems/Loral, Palo Alto, CA). The form of the in-orbit infrared calibration equation and some of the coefficients were determined from these tests. Despite the extensive testing before launch, the data from orbit revealed unforeseen performance anomalies, most notably a variation in the emissivity of the instruments' scan mirrors with east-west scan position that necessitated a change in the in-orbit calibration equation and procedures. Operational processing by the new calibration equation was initiated months after the launches of the GOES-8 and GOES-9 satellites and at different times for different instruments.
The purpose of this memorandum is to document the complete calibration processing, including the post-launch modification for the scan-mirror emissivity variation, which NOAA carries out in its ground-system computers. This is covered in sections 3-6, which follow a short description of the calibration data in section 2. Section 7 describes the digital data that users receive, which, in infrared channels, are scaled radiances, and, in visible channels, normalized instrument output relative to the level of space. Appendix A presents the procedure for users to transform the scaled radiances to physical radiances and brightness temperatures.
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Contact Michael P. Weinreb at michael.weinreb@noaa.gov
Latest Revision: July 9, 1997