Magnetic field structure through solar cycles

Details Magnetic field structure through solar cycles Magnetic field structure through solar cycles

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506.1049g&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

Sun, Magnetic Field Structure, Solar Activity

Scientific paper

We present the results of the analysis of the longitude distribution of the solar magnetic field in 21, 22 and 23 cycles of solar activity. We have used the WSO observations taken by Babcock magnetograph since 1975 to 2002. The large scale dipole and quadrupole structure are discussed. The relationship between the North and the South hemisphere as well as between the pole and equator are studied. The relation between the longitude distributions in the minimum and in the maximum of solar activity are discussed.

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