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The evolution of the polar coronal holesHe I 10830 A synoptic maps, obtained at the Kitt Peak National Observatory during 1974-1979, show that the sun's polar coronal holes have contracted significantly during 1977-1978. Prior to the accelerated increase of sunspot activity in mid-1977, the area of each polar cap was on the order of 8% of the sun's total surface area, whereas toward the end of 1978 these areas fell below 2% of the total surface area. Synoptic polar plots show that the vestigial holes had irregular shapes and were often well removed from the poles themselves. These results are consistent with the changes that one would expect when the polar magnetic fields are weakening just prior to sunspot maximum
Document ID
19800043640
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Sheeley, N. R., Jr.
(U.S. Navy, E. O. Hulburt Center for Space Research, Washington D.C., United States)
Date Acquired
August 10, 2013
Publication Date
March 1, 1980
Publication Information
Publication: Solar Physics
Volume: 65
Subject Category
Solar Physics
Accession Number
80A27810
Funding Number(s)
CONTRACT_GRANT: DPR-W14429
Distribution Limits
Public
Copyright
Other

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