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Solar large-scale positive polarity magnetic fields and geomagnetic disturbancesUnlike the negative polarity solar magnetic field large-scale regular features that correlate with enhanced solar activity regions, the positive polarity regular formations formed in the weak and old background magnetic fields seem to correlate well with geomagnetically enhanced periods of time (shifted for 4 days), which means that they seem to be the source of the quiet solar wind. This behavior of the large intervals of heliographic longitude with prevailing positive polarity fields may be followed to the end of the 18th cycle, during the declining part of the 19th cycle, and during the first half of the present 20th cycle of solar activity.
Document ID
19730002045
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Bumba, V.
(Ceskoslovenska Akademie Ved Ondrejov., United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1972
Publication Information
Publication: NASA. Ames Res. Center Solar Wind
Subject Category
Space Radiation
Accession Number
73N10772
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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