Computer Science
Scientific paper
Jun 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25..488p&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, May-June 1985, p. 488-490. In Russian.
Computer Science
Correlation Coefficients, Interplanetary Magnetic Fields, Kp Index, Solar Corona, Solar Magnetic Field, Solar Wind, Magnetic Signatures, Solar Terrestrial Interactions
Scientific paper
Two methods for describing the large-scale solar magnetic field are compared: the conventional potential method and a simplified approach involving the elementary addition of magnetic fields over the solar disk. An analysis of correlation curves obtained on the basis of Stanford magnetograph data for May-July 1979 shows that the time behavior of the NS component of the large-scale solar magnetic field calculated on the basis of the simplified method almost fully agrees with the behavior of this component as calculated on the basis of harmonic analysis. The magnetic field at different heights in the lower corona can be approximated with sufficient accuracy through the choice of an appropriate averaging.
Poniavin D. I.
Pudovkin Mikhail I.
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