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FIFI LS
| Name of Instrument: |
FIFI LS - Field Imaging Far-Infrared Line Spectrometer |
| Instrument type: |
Imaging Spectrometer
42-210 microns |
| Principal Investigator: |
A. Poglitsch |
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Contact:
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Leslie Looney: lwl@.mpg.de |
| Institute: |
Max-Planck-Institut f. extraterr. Physik
Garching, Germany
Internet: http://www.mpe.mpg.de |
Scientific/Technical Abstract:
FIFI-LS will have two separate medium resolution
(R ~ 1700) liquid helium cooled grating spectrometers with common
fore-optics feeding two large Ge:Ga detector arrays (16 x 25 pixels
each). With the two Littrow spectrometers we can simultaneously
observe an object in two spectral lines in the wavelength ranges
42 - 110 um, and 110 - 210 um, respectively, in 1st and 2nd order.
Multiplexing takes place both spectrally and spatially.
An image slicer redistributes 5 x 5 pixel spatial fields-of-view
(~ diffraction-limited in each wave band) along the 1 x 25 pixel
entrance slits of the spectrometers. Anamorphic collimator mirrors
help keep the spectrometer compact in the cross-dispersion direction. The spectrally dispersed images of
the slits are anamorphicly projected onto the detector arrays,
to independently match spectral and spatial resolution to detector
size, thus enabling instantaneously coverage over a velocity range
of ~ 1500 to 3000 km/s around selected FIR spectral lines, for
each of the 25 spatial pixels.
For calibration and flatfielding, black body calibrators
internal to the instrument are used. These
have signal levels comparable to the thermal background of the
telescope. An image rotator compensates for field rotation during
long exposures.
FIFI LS Performance Summary Instrument
sensitivity and resolution summary is provided to permit estimating
feasibility of scientific investigations.

All sensitivity and resolution data are preliminary,
and based on anticipated performance of the observatory and the
instrument. Actual performance of the SOFIA telescope and
instrument combination will be established after flight operations
begin. Telescope performance is expected to be upgraded during
the first two years, and instrument performance may be upgraded,
or additional modes or capabilities may be added.
Performance estimates given here are based on data
supplied by the instrument team. Further details and updates may
be obtained from the instrument team via the contact information
given above.
Further References:
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