Physics
Scientific paper
Jan 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..131...53w&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 131, Jan. 1991, p. 53-68. Research supported by Chinese Academy of Sciences and NNSFC.
Physics
27
Magnetic Field Configurations, Magnetic Flux, Solar Cycles, Solar Granulation, Solar Magnetic Field, Chromosphere, Magnetic Variations, Photosphere, Solar Observatories, Sunspots
Scientific paper
Several series of coordinated observations on decaying active regions and enhanced magnetic network regions on the sun were carried out jointly at Big Bear Solar Observatory and at the Huairou Solar Observing Station of the Bejing Astronomical Observatory in China. The magnetic field evolution in several regions was followed closely for three to seven days. The magnetic flux transport from the remnants of decayed active regions was studied, along with the evolution and lifetime of the magnetic network which defines the boundaries of supergranules. The magnetic flux transport in an enhanced network region was studied in detail and found to be negative. Also briefly described are some properties of moving magnetic features around a sunspot. Results of all of the above studies are presented.
Ai Guoxiang
Wang Haimin
Zirin Harold
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