Preflare conditions, changes and events

Details Preflare conditions, changes and events Preflare conditions, changes and events

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...68..217m&link_type=abstract

Solar Physics, vol. 68, Dec. 1980, p. 217-236.

Physics

67

Solar Activity, Solar Flares, Solar Magnetic Field, Solar X-Rays, Stellar Evolution, Brightness, Centimeter Waves, Circular Polarization, Magnetic Flux, Solar Corona, Solar Radio Bursts, Statistical Analysis, Sunspots

Scientific paper

The preflare conditions, changes, and events are categorized into distinct (which have direct physical connections with flares), evolutionary, and statistical. Evolutionary changes are long-term effects that may be related to the flare buildup even though these changes may occur in the absence of flares, such as the development of current sheets or strongly sheared magnetic fields, evolving magnetic features, sunspot motions, or the velocity patterns. Statistical preflare changes include distinct and evolutionary preflare changes; these events include statistically significant magnetic field properties, the brightness of active centers at various wavelengths, and increased turbulence in filaments.

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