TARGET_DESCRIPTION |
Description
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The PPR Radiometric Calibration Target (RCT) is mounted on the
spacecraft so that it is viewed by the PPR when the Galileo Orbiter
scan platform is pointed near the zero cone angle direction.
Intended primarily for calibration of the PPR thermal radiometry
bands, the RCT has a truncated conical interior with a center
cylindrical section. The interior of the target is a smooth,
specularly reflecting, black-painted surface that with the truncated
conical geometry achieves a thermal emittance of 0.998 when viewed
on axis by the PPR. Note that the end of the central cylindrical
portion of the target is not viewed by the PPR since that area is
within the central obscuration from the secondary mirror of the PPR
telescope.
The RCT is designed and mounted such that simply through passive
thermal equilibrium, it will have a temperature in the range, 125 K
to 140 K, during the Jupiter Phase of the Galileo Mission. Actual
temperature of the RCT is monitored by two platinum resistance
thermometers (PRTs) that are calibrated to an accuracy of 0.2 K.
These PRTs are connected to the PPR so that their readouts can be
included in the PPR science data stream.
Although the RCT is designed primarily to provide a target that
closely approximates a blackbody source at its monitored temperature
in order to perform inflight calibration of the PPR thermal
radiometry bands, it includes a small tungsten-filament lamp mounted
in the RCT interior so that it can be used as a radiometric and
polarimetric reference standard for the shortwave PPR bands as
well. When this lamp is commanded on for non-radiometry band
calibration, its output passes through two elliptically shaped,
plane-parallel sapphire plates mounted such that the outer surface
of the stack approximately conforms to the inner conical surface of
the RCT. This configuration provides shortwave band calibration
while having negligible effect on the thermal emittance of the RCT.
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