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High latitude solar magnetic fieldsKitt Peak magnetograms are used to measure polar magnetic fields. The polar mean absolute field increases at the same time as the polar mean field decreases. That is, the polar mean absolute field varies in phase with solar activity, in contrast to the out of phase variation of the mean polar field. It is found that the polar fields have a large bipolar component even at solar minimum, with a magnitude equal to that found at low latitudes outside the active latitude bands.
Document ID
19920059901
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Murray, Norman
(California Institute of Technology Pasadena, United States)
Date Acquired
August 15, 2013
Publication Date
April 1, 1992
Publication Information
Publication: Solar Physics
Volume: 138
Issue: 2 Ap
ISSN: 0038-0938
Subject Category
Solar Physics
Report/Patent Number
ISSN: 0038-0938
Accession Number
92A42525
Funding Number(s)
CONTRACT_GRANT: NAGW-1303
CONTRACT_GRANT: NSF AST-89-13664
Distribution Limits
Public
Copyright
Other

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