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The sunspot cycle variations of the neutral line on the source surfaceThe earlier presentation method of the sunspot cycle variations of the neutral line on the source surface by introducing the view longitude is defined. It is shown that the neutral line seen from the view longitude and the equivalent dipole (determined by Hoeksema, 1984) showed a trend of rotation throughout the sunspot cycle. However, the surface bounded by the neutral line is generally far from a circle. In fact, our combined presentation of both the equivalnet dipole and the nuetral line indicates graphically that such a simple description of the rotating (equivalent) dipole may be misleading. The concept of an inclined dipole with respect to the rotation axis may also be misleading.
Document ID
19890051550
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Saito, T.
(Tohoku Univ. Sendai, Japan)
Oki, T.
(Tohoku University Sendai, Japan)
Akasofu, S.-I.
(Tohoku Univ. Sendai, Japan)
Olmsted, C.
(Alaska, University Fairbanks, United States)
Date Acquired
August 14, 2013
Publication Date
May 1, 1989
Publication Information
Publication: Journal of Geophysical Research
Volume: 94
ISSN: 0148-0227
Subject Category
Solar Physics
Accession Number
89A38921
Funding Number(s)
CONTRACT_GRANT: NSG-7447
CONTRACT_GRANT: F19628-86-C-0030
CONTRACT_GRANT: NSF ATM-85-18512
Distribution Limits
Public
Copyright
Other

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