McIDAS Programmer's Manual
Version 2015
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GOES-7
GOES-7
produced data in two different modes:
Most GOES-7
data after 24 March 1987 (Julian day 87083) is AAA. This section documents
the mode AAA for the IR and VAS instruments. Word 52 of the area directory
contains the source type AAA.
The VAS senses
the atmosphere for a given spatial location in up to 12 different IR spectral
bands and one visible band. All or some of the IR bands may be included in
a single VAS type area. The visible, however, may be contained in a separate
area of VISR type. As a result, it may require two areas to contain the total
information transmitted by the satellite during a given time period.
GOES-7
AAA directory block
Word |
Value |
Description |
14 |
|
number
of spectral bands |
19 |
|
band
filter map; a bit is set to one for each band appearing in the area |
52 |
AAA |
image
source type; 4 bytes ASCII |
53 |
RAW |
calibration
type; 4 bytes ASCII |
GOES-7
AAA data block
The line
prefix consists of a 4-byte validity code, 512 bytes of IR common documentation,
and 116 bytes of VAS calibration information organized as follows.
Bytes |
Description |
4 |
day, yyddd |
4 |
time
of the scan, hhmmss |
4 |
scan
number (satellite coordinate line number) |
104 |
13
eight-byte groups (1 per possible band) each containing:
channel number - 2-byte binary integer (see the table on the next page)
number of spins - 2-byte binary integer
unused - 4 bytes |
The line
prefix also contains 4, 8, 12 or 16 bytes of band list information; one byte
for each band plus up to three bytes to round to the nearest whole word.
The
structure of a VAS area is complicated by two facts:
- Every line
may not contain all the spectral bands indicated in the band map (word
19 in the directory block).
- The
order of the bands may not be the same on every line.
What does
appear on a given line is indicated in the band list section, which acts
as an index for the line. Only the leftmost n bytes
of the band list contain nonzero data, with n being
the actual number of bands contained in each element of the line. The I th
byte of the band list corresponds to the I th 16-bit
pixel in each element of the line. Unused band list bytes are filled with
binary zeros; the data in the unused pixel locations may not be zero, but
in any case should be ignored.
The channel
numbers range from 1 to 38; channel 39 exists but has never been put into
service. Each is described in the table below.
Channel
|
Detector
|
Size
|
Location
|
Spectral band
|
1 |
HGCDTE |
large |
upper |
1 |
2 |
HGCDTE |
large |
upper |
2 |
3 |
HGCDTE |
large |
upper |
3 |
4 |
HGCDTE |
large |
upper |
4 |
5 |
HGCDTE |
large |
upper |
5 |
6 |
INSB |
large |
upper |
6 |
7 |
HGCDTE |
large |
upper |
7 |
8 |
HGCDTE |
large |
upper |
8 |
9 |
HGCDTE |
large |
upper |
9 |
10 |
HGCDTE |
large |
upper |
10 |
11 |
INSB |
large |
upper |
11 |
12 |
INSB |
large |
upper |
12 |
13 |
HGCDTE |
large |
lower |
1 |
14 |
HGCDTE |
large |
lower |
2 |
15 |
HGCDTE |
large |
lower |
3 |
16 |
HGCDTE |
large |
lower |
4 |
17 |
HGCDTE |
large |
lower |
5 |
18 |
INSB |
large |
lower |
6 |
19 |
HGCDTE |
large |
lower |
7 |
20 |
HGCDTE |
large |
lower |
8 |
21 |
HGCDTE |
large |
lower |
9 |
22 |
HGCDTE |
large |
lower |
10 |
23 |
INSB |
large |
lower |
11 |
24 |
INSB |
large |
lower |
12 |
25 |
HGCDTE |
small |
upper |
3 |
26 |
HGCDTE |
small |
upper |
4 |
27 |
HGCDTE |
small |
upper |
5 |
28 |
HGCDTE |
small |
upper |
7 |
29 |
HGCDTE |
small |
upper |
8 |
30 |
HGCDTE |
small |
upper |
9 |
31 |
HGCDTE |
small |
upper |
10 |
32 |
HGCDTE |
small |
lower |
3 |
33 |
HGCDTE |
small |
lower |
4 |
34 |
HGCDTE |
small |
lower |
5 |
35 |
HGCDTE |
small |
lower |
7 |
36 |
HGCDTE |
small |
lower |
8 |
37 |
HGCDTE |
small |
lower |
9 |
38 |
HGCDTE |
small |
lower |
10 |
For a given
spectral band, only one detector size is used in an area. However, two channels
representing different positions of the detector for a particular band may
appear in a single area although they may not appear on the same line. For
example, channels 8 and 20 may appear in the same area, but not channels
8 and 36.
GOES-7
AAA navigation block
Unless otherwise
noted, the words in the GOES-7 navigation block are twos-complement binary
integers.
Word |
Value |
Description |
1 |
GOES |
navigation
type (ASCII characters) |
2 |
|
satellite
ID, year, and Julian day, ssyyddd |
3 |
|
nominal
start time of the image, hhmmss |
4
- 12
4
5
6
7
8
9
10
11
12 |
1 |
orbit
parameters
orbit type
epoch date (ETIMY), yymmdd
epoch time (ETIMH), hhmmss
semimajor axis (SEMIMA), km * 100
orbital eccentricity (ECCEN) * 1000000 (unitless)
orbital inclination (ORBINC), deg * 1000
mean anomaly (MEANA), deg * 1000
argument of perigee (PERIGEE), deg * 1000
right ascension of ascending node (ASNODE), deg * 1000 |
13
- 15
13
14
15 |
|
attitude
parameters
declination of satellite axis (DECLIN), dddmmss (+=north)
right ascension of satellite axis (RASCEN), dddmmss
picture center line number (PICLIN) |
16 |
|
spin
period (SPINP); the satellite period, in microseconds, or the spin
rate in revolutions/minute |
17
- 20
17
18
19
20 |
|
frame
geometry
total sweep angle, line direction (DEGLIN), dddmmss
number of scan lines (LINTOT), nnlllll where nn is the
number of sensors and lllll is the number of scans; total
number of lines is nn * lllll
total sweep angle, element direction (DEGELE), dddmmss
number of elements in a scan line (ELETOT) |
21
- 30
21
22
23
24
25
26
27
28
29
30 |
0 |
camera
geometry
forward-leaning (PITCH), dddmmss
sideways-leaning (YAW), dddmmss
rotation (ROLL), dddmmss
reserved
east/west adjustment (IAJUST) in visible elements (+ or -)
time computed by IAJUST from the first valid landmark of the
day (IAJTIM), hhmmss
reserved
angle between VISSR and sun sensor (ISEANG), dddmmss
reserved for later implementation of *SKEW*
reserved |
31
- 38
31
32
33
34
35
36
37
38 |
|
betas
for this area
scan line of the first beta
time of the first beta scan line (beginning), hhmmss
time of the first beta scan line (continued), milliseconds*10
beta count 1
scan line of the second beta
time of the second beta scan line (beginning), hhmmss
time of the second beta scan line (cont.), milliseconds*10
beta count 2 |
39-128
39
40
41-120
121-128 |
|
gammas
for this area
gamma, element offset * 100; this is the nominal offset at
time zero of this day
gamma-dot, element drift per hour * 100
reserved
memo; up to 32 ASCII characters of comments |
GOES-7
AAA calibration block
The calibration
block is composed of the following data.
Word |
Value |
Description |
1 |
|
sensor
source number |
2 |
|
date, yyddd |
3 |
|
time, hhmmss |
4
- 9 |
|
radiance
equation coefficients, array IAB(2,38) |
80
- 117 |
|
radiance
equation coefficients scale factors, IFAB(38) |
118-128 |
0 |
|
Transforming
the VAS raw IR values into brightness temperatures is accomplished via the
intermediate computation of calibrated VAS radiances. The array IAB contains
two coefficients for each of the 38 channels; IFAB contains one scale factor
for each channel.
If the channel
is ICHAN, compute the radiance for the raw value P using:
AB1 = IAB (1,ICHAN)
AB2 = IAB (2,ICHAN)
FAB = 2.**(15-IFAB (ICHAN))
R = (AB2 * P /32.
- AB1) / FAB
The raw value P is
divided by 32 because the data is stored as 15-bit numbers, but the coefficients
expect 10-bit numbers.
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