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Solar cycle changes in the polar solar windIt is noted that although the 11 year solar cycle was first recognized in 1843, it is still only poorly understood. Further, while there are satisfactory models for the magnetic variations, the underlying physics is still obscure. New observations on the changing three-dimensional form of the solar wind are presented which help relate some of the modulations observed in geomagnetic activity, the ionosphere, and the flux of galactic cosmic rays.
Document ID
19800058887
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Coles, W. A.
(California Univ. La Jolla, CA, United States)
Rickett, B. J.
(California Univ. La Jolla, CA, United States)
Rumsey, V. H.
(California Univ. La Jolla, CA, United States)
Kaufman, J. J.
(California Univ. La Jolla, CA, United States)
Turley, D. G.
(California, University La Jolla, Calif., United States)
Ananthakrishnan, S.
(Tata Institute of Fundamental Research Ootacamund, India)
Armstrong, J. W.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Harmons, J. K.
(Arecibo Observatory Arecibo, P.R., United States)
Scott, S. L.
(Owens Valley Radio Observatory Big Pine, Calif., United States)
Sime, D. G.
(High Altitude Observatory Boulder, Colo., United States)
Date Acquired
August 10, 2013
Publication Date
July 17, 1980
Publication Information
Publication: Nature
Volume: 286
Subject Category
Solar Physics
Report/Patent Number
AFGL-TR-81-0113
AD-A099231
Accession Number
80A43057
Funding Number(s)
CONTRACT_GRANT: F19628-77-C-0161
CONTRACT_GRANT: NSF ATM-78-6770
Distribution Limits
Public
Copyright
Other

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