Physics
Scientific paper
Jan 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...75..361m&link_type=abstract
Solar Physics, vol. 75, Jan. 1982, p. 361-375.
Physics
9
Interplanetary Magnetic Fields, Magnetic Poles, Polarity, Solar Cycles, Anisotropy, Coronal Holes, Current Sheets, Solar Activity Effects, Tables (Data)
Scientific paper
A study of the predominant interplanetary magnetic field (IMF) polarity is made for the years 1957-1977. An examination of the mean positive and negative sector width for time periods (semesters) for which the earth was in northern and southern heliolatitudes shows that the predominant polarity for every semester follows, up to a certain extent, the Rosenberg-Coleman effect. The statistical support, however, is not satisfactory. It is noted that the same conclusion was reached by a similar study of data grouped over various phases of the solar cycle. The relative frequency of positive (negative) IMF polarity days shows that the general pattern of the mean IMF has a tendency to reoccur in the homologous (corresponding) phases of different solar cycles.
Moussas Xenophon
Tritakis B.
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