A quasi-Complex of Activity distribution for the regions of flare activity

Details A quasi-Complex of Activity distribution for the regions of flare activity A quasi-Complex of Activity distribution for the regions of flare activity

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980acasn..21..349c&link_type=abstract

Acta Astronomica Sinica, vol. 21, Dec. 1980, p. 349-353. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

Radiative Lifetime, Solar Activity Effects, Solar Flares, Solar Magnetic Field, Data Acquisition, Long Term Effects, Solar Rotation, Spatial Distribution

Scientific paper

By tracing the positions of the regions of flare activity from January, 1970 to December, 1975, it is proposed that these regions exhibit a regional distribution of quasi-CA (complex of activity) on the surface. 95% active regions were distributed in 21 quasi-CA districts. The lifetime of quasi-CA is long and some may survive to over thirty rotations. After it has disappeared, and a quiet period of several (up to ten) more rotations has elapsed, some new regions can be activated in these districts. Therefore, it may provide an important parameter for the long-term prediction of solar flares.

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