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SOFIA: Stratospheric Obsrvatory for Infrared Astronomy

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SOFIA Rollout at L3 Communications in Waco, Texas-- September 2006. 3 ... angular resolution than Kuiper Airborne Observatory or Spitzer Space Telescope. ... – PowerPoint PPT presentation

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Title: SOFIA: Stratospheric Obsrvatory for Infrared Astronomy


1
SOFIA Stratospheric Obsrvatory for Infrared
Astronomy
2

SOFIA Rollout at L3 Communications in Waco,
Texas-- September 2006
3
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4
HAWCHigh-resolution Airborne Wideband Camera
  • Facility far infrared camera for SOFIA spectral
    range 40-300 µm
  • Built by University of Chicago
  • Four filters at 53, 88, 155, and 215 µm,
    0.1ltDl/llt0.2
  • 12 x 32 Pop-up Detectors (PUD) array cooled to
    0.2K with adiabatic demagnetization refrigerator
    (ADR)
  • Design optimized to give the highest possible
    angular resolution at each wavelength
  • Science formation and evolution of stars,
    galaxies, and planetary systems physics of dust
    and the interstellar medium
  • Status in assembly and testing phase at
    University of Chicago

5
SOFIAs angular resolution is limited by
atmospheric turbulence at short wavelengths and
by diffraction at long wavelengths.
6
HAWC/SOFIA gt Goal is sharpest possible images of
the far-infrared universe. Three times better
angular resolution than Kuiper Airborne
Observatory or Spitzer Space Telescope.
Science example formation of massive stars in
the Orion Molecular Cloud
7
Pop-up Detector Array
folded silicon bolometers
12 32 array
row of 32 folded bolometers
JFET modules
8
Assembly of HAWC far infrared detector at Goddard
Space Flight Center . 1x32 rows of detectors are
stacked into a 12x32 array and connected to
electrical fanout boards via microbridge thermal
isolators.
9
Flight Cryostat
Vapor-Cooled Shields
Fore-optics assembly images telescope pupil onto
cold Lyot stop
HTS System kinematic support and thermal
isolation of helium-cooled optics assembly via
Kevlar straps
Opto-Mechanical System (OMS) Four
interchangeable lenses with broadband filters,
eight interchangeable Lyot stops and/or filters
in cold pupil plane.
Detector
Adiabatic Demagnetization Refrigerator (ADR)
cools detector to 200 mK
Liquid Helium Reservoir capacity 60 liters
10
Adiabatic Demagnetization Refrigerator Cools
detector array to 200mK
11
Assembly of HAWC flight cryostat
12
University of Chicago astronomers pioneered
airborne infrared astronomy with 30-cm Lear Jet
telescope during 1970s.
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