1. INTRODUCTION
The National Oceanic and Atmospheric Administration (NOAA) operates a system
of Geostationary Operational Environmental Satellites (GOES) to provide frequent
visible and infrared images of the Earth as well as quantitative meteorological
data products, such as estimates of atmospheric temperature and moisture
profiles, winds, and precipitation. The imagery is well-known to the general
public through televised weather reports. The GOES-8 and -9 satellites, launched
on April 13, 1994, and May 23, 1995, respectively, are currently stationed at
36,000 km above the equator at 75W and 135W longitudes, respectively. Both carry
an Earth-atmosphere imager and an atmospheric sounder1-3. These instruments
observe the Earth in a total of 24 spectral intervals ("channels") at
wavelengths between 0.6 µm and 14.7 µm. The imager makes observations in five
channels (Table 1), which are isolated by stationary filters in its optical
chain. Each channel utilizes a separate linear north-south array of
detectors--eight detectors in channel 1, two in channels 2, 4, and 5, and one
in
channel 3. The sounders observe in 19 spectral intervals (Table 2).
Table 1. Characteristics of imager channels
| 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 |
Table 2. Characteristics of imager channels
| 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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