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Cosmic rays and the dynamic balance in the Large Magellanic CloudPresent and future measurement of the Large Magellanic Cloud (LMC) particularly in the radio and high energy gamma ray range offer the possibility of understanding the density and distribution of the cosmic rays in a galaxy other than our own and the role that they play in galactic dynamic balance. After a study of the consistency of the measurements and interpretation of the synchrotron radiation from our own galaxy, the cosmic ray distribution for the LMC is calculated under the assumption that the cosmic ray nucleon to electron ratio is the same and the relation to the magnetic fields are the same, although the implications of alternatives are discussed. It is seen that the cosmic ray density level appears to be similar to that in our own galaxy, but varying in position in a manner generally consistent with the concept of correlation with the matter on a broad scale.
Document ID
19930039453
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Fichtel, Carl E.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Ozel, Mehmet E.
(Cukurova Univ. Adana, Turkey)
Stone, Robert G.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1990
Publication Information
Publication: In: Observatories in earth orbit and beyond (A93-23401 07-89)
Publisher: Kluwer Academic Publishers
Subject Category
Space Radiation
Accession Number
93A23450
Distribution Limits
Public
Copyright
Other

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