June-July 1974 proton-flare region. IV - The dynamics of the local magnetic field evolution during the proton-flare events rotation

Details June-July 1974 proton-flare region. IV - The dynamics of the local magnetic field evolution during the proton-flare events rotation June-July 1974 proton-flare region. IV - The dynamics of the local magnetic field evolution during the proton-flare events rotation

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982baicz..33..281b&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin, vol. 33, no. 5, 1982, p. 281-285.

Astronomy and Astrophysics

Astronomy

5

Solar Flares, Solar Magnetic Field, Solar Protons, Sunspots, Magnetic Flux, Polarity

Scientific paper

The dynamics of the day to day evolution of the June-July 1974 proton-flare region's local magnetic field, composed originally of at least two individual local fields, are analyzed, and the development of the magnetic centers of activity of the proton-flare local magnetic field is investigated. Results show that the development of the new magnetic fluxes can be related to two main and at least one secondary center of activity. It is indicated that one of the main reasons for the changes of the observed field topology is the tendency of the complex magnetic field to form one simple bipolar field, properly inclined toward the equator. During these changes of the field topology, the positive field of the eastern region extended toward the west to join the same polarity field of the western region and became the main leading field. The western negative polarity field shifted towards the east to join the eastern field of like polarity which took over the role of the main following field.

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