Weak solar fields and their connection to the solar cycle

Details Weak solar fields and their connection to the solar cycle Weak solar fields and their connection to the solar cycle

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..110..101z&link_type=abstract

(Solar Cycle Workshop, 1st, Pasadena, CA, Aug. 17-20, 1986) Solar Physics (ISSN 0038-0938), vol. 110, no. 1, 1987, p. 101-107.

Physics

60

Bipolarity, Magnetic Field Configurations, Solar Cycles, Solar Magnetic Field, Steady State, Sunspots, Magnetic Flux, Magnetic Signatures

Scientific paper

Videomagnetograph observations of the weak solar magnetic fields are discussed. Intranetwork (IN) elements are found to emerge in bipolar form, but to flow in a random pattern rather than toward the network elements. Merging of IN fields is found to be more important than the ephemeral regions as a source of new network elements. Arguments for and against the hypothesis that all solar fields are intrinsically strong are considered. It is noted that reconnection and merging of magnetic fields take place continually under the conditions presently examined.

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