Investigation of the solar differential rotation by hydrogen filaments in 1976 1986

Details Investigation of the solar differential rotation by hydrogen filaments in 1976 1986 Investigation of the solar differential rotation by hydrogen filaments in 1976 1986

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..141..267j&link_type=abstract

Solar Physics, Volume 141, Issue 2, pp.267-274

Physics

14

Scientific paper

Based on observational data on chromosphere filaments, certain characteristics of solar differential rotation during solar activity cycle No. 21 are determined at Abastumani Astrophysical Observatory. In the northern hemisphere of the Sun, propagation of a quasi-bi-annual impulse of the rotation residual from high latitudes to the equator is found in 1979 1981. It is supposed that this phenomenon might be related to the polarity reversal in the northern hemisphere of the Sun in 1981.0.

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