NICMOS Dewar
The NICMOS dewar (view schematic) is
used to cool the detectors and
optical elements of the three NICMOS cameras. Initially
following installation onboard
HST during Servicing Mission 2 (SM2),
February 11, 1997, the
dewar contained solid Nitrogen encased in
an Aluminum foam. However, due to a thermal
short following SM2, the solid Nitrogen was
depleted in January 1999. A cryocooler,
cirulating a cold Neon gas, will be installed
on NICMOS to cool the detectors during
SM3B.
Prior to the SM2 launch, an extensive ground testing program
was executed, during which
the NICMOS dewar was filled with about 240 pounds of liquid nitrogen. The
nitrogen was then
solidified by passing cold helium gas through a coil located at the aft end of
the dewar. This reduced the temperature of the nitrogen to about 40 K. During
testing and storage,
passive heat
inputs caused the block of solid nitrogen to slowly warm up - an expected
behavior. To avoid
reaching the triple point at about 63 K, the block was recooled approximately
every 6-8 weeks,
again using cold Helium gas circulating through the aft end cooling coil. During
this process,
nitrogen gas froze onto the cooling coil. This reduced the vapor pressure at the
aft end, effectively
pumping gas from the warmer fore end to the aft.
As the dewar was allowed to warm up, the ice at the aft end
expanded, pushing into the interior
surfaces of the dewar and deforming it. By mid-1996 the three cameras in NICMOS
were no
longer parfocal although there were good reasons to expect that they would
return to a nearly
parfocal state after a fraction of the nitrogen had evaporated on orbit. At that
time a total
deformation of about 4 mm had been observed and steps were taken to assure that
the dewar
remained flight worthy and that subsequent recooling Cycles did not stretch the
dewar further.
After NICMOS was installed in HST, the dewar was planned to
warm up to about 57 K. This high a
temperature was never
allowed to be reached during ground testing. The ice expansion caused by this
temperature
increase resulted in an additional dewar deformation, to the extent that one of
the (cold) optical
baffles made mechanical contact with the warmer vapor-cooled shield (VCS). The
resulting
heat flow caused the ice to warm up even more, to about 60 K, which in turn
deformed the dewar
more. The thermal short increased the heat flux into the inner shell by a factor
of 2.5 and thus reduced the lifetime of NICMOS from 4.5 to 2 years. The cryogen
depleted in January, 1999, and NICMOS was unavailable for science until the
installation of NCS in March 2002.
In March 2002, the NCS was successfully installed on the
NICMOS, and the instrument is now
performing even better than it did during Cycle 7. Now operating at a slightly
warmer temperature,
77.1 K, the Instrument is more sensitive than it was during Cycle 7 and the
temperature is also
more constant. Furthermore, the focii for all three cameras have remained
stable, and the NIC3
focus has moved in the positive direction relative to its Cycle 7 position, so
as to be nearly
in focus! Details about the operation of the NICMOS under NCS, as well as
recommended strategies
for observing proposals can be found in the Cycle
17 Instrument Handbook.
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