The relationship between the interplanetary magnetic field inhomogeneous structure and the distribution of large-scale magnetic fields in the photosphere (1969-1975)

Details The relationship between the interplanetary magnetic field inhomogeneous structure and the distribution of large-scale magnetic fields in the photosphere (1969-1975) The relationship between the interplanetary magnetic field inhomogeneous structure and the distribution of large-scale magnetic fields in the photosphere (1969-1975)

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph..102..191p&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 102, no. 1-2, Dec. 1985, p. 191-201.

Physics

1

Interplanetary Magnetic Fields, Magnetic Field Configurations, Nonuniform Magnetic Fields, Photosphere, Solar Magnetic Field, Asymmetry, Inhomogeneity, Long Term Effects, Mapping, Solar Activity Effects

Scientific paper

For the period 1969-1975, a study has been made of the dependence of the interplanetary magnetic field structure on the distribution and evolutionary properties of solar magnetic fields. By direct comparison of a sequence of synoptic charts of the photospheric magnetic field with the interplanetary magnetic field, and by applying the method of correlation analysis, it is shown that areas with an unstable polarity of the interplanetary magnetic field have corresponding regions with a complicated inverse polarity line that forms either narrow gulfs and islands against a background of dominant polarity, or of bipolar magnetic regions and their clusters. At the time of reconstruction of the photospheric magnetic field, the correlation between the photospheric and interplanetary magnetic-field-element-distributions worsens. An asymmetry of the correlation between the interplanetary and photospheric magnetic field structures of different hemispheres is found. During the period of study, the interplanetary field structure shows a better correlation with the distribution of the photospheric magnetic field at middle and lower latitudes (0-40 deg) of the southern hemisphere.

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