IRAS Explanatory Supplement
XI. Known Processing Anomalies
F. Artifacts in the Digital Image Data Base
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The final calibration corrections for baseline and scale
factor in the 16.5° image digital data base delivered in
November 1984 (third HCON coverage only) were based on the Zodiacal
History file. There was insufficient time before the delivery
date to perform the corrections properly on the time ordered data
and reassemble the high resolution maps. As a result, the 2' digital
data show a patchwork structure of 30' squares which varies in
intensity from one part of the sky to another. The maximum discontinuity
across the edge of one of the squares amounts to about 5 digitization
levels of the satellite's
electronics in all bands
(Section II.C) regardless of the instantaneous
sky brightness. This translates to maximum jumps of about 0.9,
2.0, 0.5 and 1.0 MJy sr-1 at 12, 25, 60 and 100 µm,
respectively.
The problem should be of little concern in high brightness regions
such as the Galactic plane but may compromise the data for some
purposes in low brightness regions near the Ecliptic and Galactic
poles. In most cases the patchwork amplitude is smaller than the
residual striping left by the flat fielding procedure.
No attempt was made to smooth out the discontinuities. A
number of fields where the problem was most severe were deleted
and are listed in
Table XI.F.1.
The calibration of the third coverage
will be corrected properly and a complete data set reissued.
The photographic data products released in November, 1984 do not
suffer from the problem because no corrections were applied to
these data as discussed in
Section X.D.3. The first and second
HCON coverages as well as the reprocessed third HCON will be properly
corrected.
Fields Deleted from 3rd HCON
Table XI.F.1
| 7 | 18 | 19 | 20 | 21 | 22 |
| 23 | 24 | 36 | 43 | 44 | 56 |
| 58 | 82 | 92 | 116 | 127 | 140 |
| 141 | 170 | 173 | 185 | 186 | 187 |
| 188 | 190 | 191 | 192 | 201 | 203 |
| 205 | 209 | 210 | - | - | - |
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