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A pulsar emission model - Observational testsThe usual model for coherent radio emission, curvature radiation from bunches, is applied here to a modified 'hollow cone' model in which only one or a few geometrically fixed flux tubes are radiating into a fan beam. The way that the model handles the basic problems of sufficient radio power output, reasonable spectrum, and narrow pulses as well as the secondary issues of orthogonal mode changing, complex pulse profiles is addressed. Issues that seem more model-dependent, including flux tube scales, nulling, self-absorption, drifting subpulses, and radius-to-frequency mapping, are examined by considering a specific global model.
Document ID
19880031870
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Michel, F. Curtis
(California Institute of Technology Pasadena, United States)
Date Acquired
August 13, 2013
Publication Date
November 15, 1987
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 322
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
88A19097
Funding Number(s)
CONTRACT_GRANT: NSF PHY-85-05682
CONTRACT_GRANT: NSF PHY-86-04197
CONTRACT_GRANT: NSF AST-85-11709
CONTRACT_GRANT: NAGW-379
Distribution Limits
Public
Copyright
Other

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