Magnetic fields of solar prominences: strength and latitude distribution.

Details Magnetic fields of solar prominences: strength and latitude distribution. Magnetic fields of solar prominences: strength and latitude distribution.

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989bsold..11...98k&link_type=abstract

Byulletin Solnechnye Dannye Akademie Nauk USSR, No. 1989/11 p. 98 - 102

Mathematics

Probability

1

Solar Prominences: Magnetic Fields

Scientific paper

According to the data obtained by a Nikolsky-type magnetograph during 1979 - 1986 there are two maxima in histograms "occurrence-B∥": O - 21 G and 27 - 36 G. The probability of the minimum between these maxima is equal to 82%. The first maximum may be divided into three distributions with peaks at 8, 15 and 20 G. The second maximum refers to active latitude prominences. The major part of the data (80%) belongs to the pre-minimum and minimum epochs. For this period the average latitude of prominence formation is less than 20°. The authors believe that the peak at 15 G characterizes the critical field strength of prominence formation.

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