Preferred Bartels days of high speed solar wind streams - an update

Details Preferred Bartels days of high speed solar wind streams - an update Preferred Bartels days of high speed solar wind streams - an update

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..122..187r&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 122, no. 1, 1989, p. 187-189.

Physics

5

Solar Cycles, Solar Rotation, Solar Wind Velocity, Interplanetary Magnetic Fields, Solar Flares

Scientific paper

Comparison of distribution of solar wind streams as a function of
Bartels rotation days for two successive epochs indicates several
significant differences. These are likely to be due to the differing
nature of IMF and solar wind in the two solar cycles 20 and 21.

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