Other
Scientific paper
Aug 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984sci...225..793v&link_type=abstract
Science (ISSN 0036-8075), vol. 225, Aug. 24, 1984, p. 793-800. Research supported by the National Geographic Society.
Other
12
Magnetic Stars, Solar Activity, Stellar Activity, Stellar Magnetic Fields, Chromosphere, Chronology, H Lines, Histories, K Lines, Periodic Variations, Solar Rotation, Stellar Models, Sunspots
Scientific paper
The solar magnetic field, when carried into interplanetary space by the solar wind, creates changes in the earth's magnetosphere and variations in the galactic cosmic ray particle flux incident on the earth's upper atmosphere. Observational data accumulated over several centuries have indicated that the solar magnetism exists and varies in a globally organized pattern that is coupled to the sun's rotation. Wilson (1966, 1981) has demonstrated that analogs of solar activity exist and can be studied in many other dwarf stars, so that knowledge of the precise rates of rotation of stars under investigation can increase understanding of the origins of solar activity in particular and stellar activity in general.
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