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Ultrasoft X-ray Background Observations of the Local Interstellar MediumPreliminary results from a May 8, 1984 sounding rocket survey of the soft X-ray background are presented. The X-ray detectors are sensitive to X-rays in three soft X-ray bandpasses: 80 to 110 eV, 90 to 188 eV, and 284 to 532 eV (at 20% of peak response). The lowest energy X-rays in this range have a mean free path of order 10 to the 19th power/sq cm and provide information about the local interstellar medium. The count rate in the 80 to 110 eV energy band (the Be band) tracks the 90 to 188 (eV band (the B band) very well, indicating that the same approx. 1 million degree gas that is responsible for the B band emission may be responsible for the bulk of the Be band X-rays as well.
Document ID
19850007262
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Sanders, W. T.
(Wisconsin Univ. Madison, WI, United States)
Snowden, S. L.
(Wisconsin Univ. Madison, WI, United States)
Bloch, J. J.
(Wisconsin Univ. Madison, WI, United States)
Juda, M.
(Wisconsin Univ. Madison, WI, United States)
Jahoda, K. M.
(Wisconsin Univ. Madison, WI, United States)
Mccammon, D.
(Wisconsin Univ. Madison, WI, United States)
Date Acquired
August 12, 2013
Publication Date
November 1, 1984
Publication Information
Publication: NASA. Goddard Space Flight Center Local Interstellar Medium, No. 81
Subject Category
Astrophysics
Accession Number
85N15571
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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