Physics
Scientific paper
Jul 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980rspta.297..521h&link_type=abstract
(Royal Society, Discussion on the Sun and the Heliosphere, London, England, Apr. 3, 4, 1979.) Royal Society (London), Philosophi
Physics
2
Coronal Holes, Solar Magnetic Field, Solar Terrestrial Interactions, Solar Wind, Geomagnetism, Interplanetary Magnetic Fields, Magnetic Disturbances, Twenty-Seven Day Variation
Scientific paper
One of the long-standing problems of solar-terrestrial physics is examined: the connection between geomagnetic disturbances recurring within the 27 day synodic solar rotation period and plasma streams emitted from particular regions on the sun (so-called M-regions). The solar sources of these streams have been identified as large-scale coronal regions of open, diverging magnetic fields and abnormally low particle densities, observed as coronal holes. The temporal evolution of holes and streams seems to reflect the evolution of the large-scale solar magnetic fields; the observed spatial pattern of holes suggests a grand three-dimensional structure of solar wind flow and interplanetary magnetic fields organized by a near-equatorial neutral sheet
Holzer Thomas Edward
Hundhausen Arthur J.
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