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Multicomponent analysis of total COS-B gamma-ray data at intermediate lattitudesThe final COS-B database was used to study the gamma ray emission in the latitude range 10 deg /b/ 20 deg in terms of a four component model. The emissivity spectrum of the local interstellar medium is derived and compared with that found in previous studies. The intensity-Compton component is determined from the fitting procedure and is in good agreement with theoretical values.
Document ID
19850025678
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Strong, A. W. (Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Bloemen, J. B. G. M. (Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Hemsen, W. (Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Mayer-Hasselwander, H. A. (Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 1
Subject Category
Space Radiation
Report/Patent Number
OG-3.1-3
Report Number: OG-3.1-3
Accession Number
85N33991
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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