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The submillimeter wave astronomy satelliteThe Submillimeter Wave Astronomy Satellite (SWAS) selected for flight as part of the Small Explorer Program is described. SWAS consists of a 55 by 71 cm near optical quality off axis primary mirror, two heteorodyne radiometers with Schottky barrier diode mixers, and a single broadband (1.4 GHz) Acousto Optical Spectrometer (AOS). SWAS primary objective is to conduct a high spectral resolution survey of galactic molecular clouds in low lying transitions of water, molecular oxygen, atomic carbon and isotopic carbon monoxide. These species are crucial in gaining a better understanding of the chemistry and cooling of dense molecular clouds.
Document ID
19910012712
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Melnick, Gary J.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA., United States)
Dalgarno, A.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA., United States)
Erickson, N. R.
(Massachusetts Univ. Amherst., United States)
Fazio, G. G.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA., United States)
Goldsmith, P. F.
(Massachusetts Univ. Amherst., United States)
Harwit, Martin
(National Air and Space Museum Washington, DC., United States)
Hollenbach, D. J.
(NASA Ames Research Center Moffett Field, CA., United States)
Koch, D. G.
(NASA Ames Research Center Moffett Field, CA., United States)
Neufeld, David A.
(Johns Hopkins Univ. Baltimore, MD., United States)
Schieder, R.
(Cologne Univ. Germany, F.R. , United States)
Date Acquired
September 6, 2013
Publication Date
December 1, 1990
Publication Information
Publication: ESA, From Ground-Based to Space-Borne Sub-mm Astronomy
Subject Category
Spacecraft Design, Testing And Performance
Accession Number
91N22025
Distribution Limits
Public
Copyright
Other
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