Observations of the solar mean magnetic field at the Sayan Observatory during 1982 1984

Details Observations of the solar mean magnetic field at the Sayan Observatory during 1982 1984 Observations of the solar mean magnetic field at the Sayan Observatory during 1982 1984

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..114..147g&link_type=abstract

Solar Physics, Volume 114, Issue 1, pp.147-163

Physics

Scientific paper

This paper presents some results of observations of the mean magnetic field of the Sun as a star (SMMF) at the Sayan Observatory during 1982 1984. A description of the instrument is given, as well as some major points in the technique of data acquisition and treatment such as calibration, zero-level control, etc. The comparison of a new SMMF series with observations from the Wilcox Solar Observatory showed a high correlation between the two series (g9 = 0.88) but with a rather great difference in amplitudes. We discuss time variations of SMMF, both long-term caused by the magnetic field evolution with the activity cycle and those of shorter time-scales caused by solar rotation.

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