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Diffuse galactic emissionA very large portion of the observed diffuse X-ray intensity below 1 keV is of galactic origin. Observational evidence indicates that the radiation is truly diffuse, is from interstellar gas near 1 million K that is overpressured relative to the nominal interstellar pressure, and is probably from regions close to the solar system.
Document ID
19780064819
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Kraushaar, W. L. (Wisconsin, University Madison, Wis., United States)
Date Acquired
August 9, 2013
Publication Date
May 1, 1978
Subject Category
Space Radiation
Meeting Information
Meeting: Plenary Meeting
Location: Innsbruck
Country: Austria
Start Date: May 29, 1978
End Date: June 10, 1978
Sponsors: COSPAR
Accession Number
78A48728
Funding Number(s)
CONTRACT_GRANT: NAS5-22410
CONTRACT_GRANT: NGL-50-002-044
Distribution Limits
Public
Copyright
Other

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