On the measurements of the magnetic disbalance of the Sun

Details On the measurements of the magnetic disbalance of the Sun On the measurements of the magnetic disbalance of the Sun

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002kfnt...18..205k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 18, no. 3, p. 205-216

Computer Science

4

Scientific paper

The 1968-2000 time sequence of the mean magnetic field of the Sun as a star is analysed (MMF, more than 12 thousands of daily measurements). It is shown that nominally -- on the basis of the total MMF measurements set -- the southern polarity of the magnetic field predominates on the Sun, with the average value -1.9± 1.1 μ T (the magnetic asymmetry is significant at about 91%; however, its instrumental origin cannot be completely excluded). The MMF changes with the 22-year cycle, so that its predominant polarity tends to coincide with that of the Sun's northern pole; the mean amplitude of this variation is equal to 6 μ T. It is concluded that the northern pole polarity tends to "determine" the dominant polarity of solar background fields for the most area of the photosphere (at heliolatitudes higher than -500).

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