Morphological and rotational characteristics of the active regions of strong proton flares.

Details Morphological and rotational characteristics of the active regions of strong proton flares. Morphological and rotational characteristics of the active regions of strong proton flares.

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996acaps..16..314z&link_type=abstract

Acta Astrophys. Sin., Vol. 16, No. 3, p. 314 - 322

Astronomy and Astrophysics

Astrophysics

Solar Active Regions: Morphology, Sunspot Groups: Rotation

Scientific paper

The results of this study indicate that before and after proton flares, clockwise and counterclockwise rotation of the sunspot groups are early or late exist for the same sunspot group on the solar disk. The common characteristics of the active regions of the strong proton flares are shown. If the activity of the above active regions is already stronger when they move to the west of the sun, then when they turn to the western limb and back of the sun or again cross the solar disk, will produce more large proton flares.

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