Physics
Scientific paper
Jun 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...62..277l&link_type=abstract
Solar Physics, vol. 62, June 1979, p. 277-303.
Physics
5
Interplanetary Magnetic Fields, Photosphere, Solar Magnetic Field, Spatial Distribution, Cross Correlation, Data Reduction, Long Term Effects, Magnetic Field Configurations, Magnetic Signatures, Polarity
Scientific paper
The spatial organization of the observed photospheric magnetic field as well as its relation to the polarity of the IMF have been studied using high resolution magnetograms from the Kitt Peak National Observatory. Systematic patterns in the large scale field are due to contributions from both concentrated flux and more diffuse flux. The polarity of the photospheric field, determined on various spatial scales, correlates with the polarity of the IMF. Analyses based on several spatial scales in the photosphere suggest that new flux in the interplanetary medium is often due to relatively small photospheric features which appear in the photosphere up to one month before they are manifest at the earth.
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