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..267d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 141, no. 2, p. 267-274.

Physics

8

Chromosphere, Solar Activity, Solar Atmosphere, Solar Prominences, Solar Rotation, Angular Velocity, H Alpha Line, Solar Cycles

Scientific paper

The solar differential rotation by H-alpha filaments is investigated based on Abastumani Astrophysical Observatory observational data on chromospheric filaments according to the 'Solar Service' program in 1976-1986. Propagation of a quasi-biannual impulse of the rotation residual from high latitudes to the equator is found in the solar northern hemisphere for 1979-1981. It is suggested that this phenomenon may be related to the polarity reversal in the solar northern hemisphere in 1981.0.

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