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SOFIA: Stratospheric Observatory for Infrared AstronomySOFIA will be a three meter class telescope operating in a Boeing 747, offering astronomers routine access to infrared wavelengths unavailable from the ground, and with the means to observe transient astronomical events from anywhere in the world. The concept is based on 15 years of experience with NASA's Kuiper Airborne Observatory (KAO), which SOFIA will replace in the mid 1990's. SOFIA's wavelength range covers nearly four decades of the electromagnetic spectrum: from the visible, throughout the infrared and submillimeter, to the microwave region. Relative to the KAO, SOFIA will be roughly ten times more sensitive for compact sources, enabling observations of fainter objects and measurements at higher spectral resolution. Also, it will have three times the angular resolving power for wavelengths greater than 30 microns, permitting more detailed imaging at far infrared wavelengths.
Document ID
19900012030
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Erickson, E. F.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
September 6, 2013
Publication Date
October 1, 1989
Publication Information
Publication: Proceedings of the Third Infrared Detector Technology Workshop
Subject Category
Astronomy
Accession Number
90N21346
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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