A consideration of the solar cycle in the light of the behavior of the large active regions

Details A consideration of the solar cycle in the light of the behavior of the large active regions A consideration of the solar cycle in the light of the behavior of the large active regions

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.220..231g&link_type=abstract

In ESA The Hydromagnetics of the Sun p 231-232 (SEE N85-25091 14-92)

Physics

Magnetic Flux, Solar Activity, Solar Cycles, Data Smoothing, Magnetic Equator, Solar Flux, Solar Magnetic Field

Scientific paper

The solar cycle was studied by considering only the large active regions (AR), with small region data being ignored. Results show that at birth almost all the large AR display the correct inclination (p-part at lower latitude) while the small AR show random behavior. The maximum latitude attained by the large AR is lower by 10 deg than that of the small ones. The overlapping of contiguous cycles disappears when only large AR are considered. The number distribution of large AR differs from the Wolf number, which mixes large and small AR.

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