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Analytic limits on the forms of spectra possible from optically thin collisional bremsstrahlung source modelsThe constraints on hard X-ray bremsstrahlung spectral forms required in order for them to correspond to physically acceptable (nonnegative) electron distributions in thin-target, thick-target, and thermal source models are discussed. The extent to which various spectra can be attributed to the different models is examined, showing that many possible spectra cannot be described by all, or in some cases, any of the models. It is shown that for any bremsstrahlung cross section, the thick-target and thermal models require that successively higher derivatives of the thin-target constraint have the appropriate sign. It is found that thermal models are the most restrictive, and that thin-target models are the least restrictive. Explicit analytic constraint expressions are derived for all three cases for the Kramers cross section and examples of acceptable and unacceptable spectra are given. Application of these criteria to the testing and exclusion of models is discussed.
Document ID
19880060296
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Brown, John C.
(Glasgow, University United Kingdom)
Emslie, A. Gordon
(Alabama, University Huntsville, United States)
Date Acquired
August 13, 2013
Publication Date
August 1, 1988
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 331
ISSN: 0004-637X
Subject Category
Solar Physics
Accession Number
88A47523
Funding Number(s)
CONTRACT_GRANT: NAG8-52
CONTRACT_GRANT: NAG5-500
CONTRACT_GRANT: NSF AST-83-51058
CONTRACT_GRANT: NSF ATM-85-05475
CONTRACT_GRANT: NAGW-294
Distribution Limits
Public
Copyright
Other

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