Connection Between the Appearance of Flares and the Development of Sun Spots

Details Connection Between the Appearance of Flares and the Development of Sun Spots Connection Between the Appearance of Flares and the Development of Sun Spots

Jan 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000lapa....2...31s&link_type=abstract

Warta LAPAN, vol. 2, p. 31

Physics

Sunspots, Magnetic Flux, Solar Flares, Classifications, Magnetic Fields

Scientific paper

Each time condition of the development of sunspot during its life can be classified into several classes of Zurich sunspot. The polarization of magnetic field is constant during sunspot appearing from east direction until disappear in the west direction. Magnetic field intensity around the peak of its life is almost constant. Addition and substraction of the area and the number of sunspot are irregular. Flares will appear on and surrounding the sunspot area and have various number and classification for each sunspot group, although the sunspot groups are in the same class.

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