Physics
Scientific paper
Sep 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..117..243m&link_type=abstract
(Solar Cycle Workshop, Meeting, 2nd, Lake Tahoe, CA, May 1987) Solar Physics (ISSN 0038-0938), vol. 117, no. 2, 1988, p. 243-259
Physics
114
Ephemerides, Magnetic Field Configurations, Solar Activity, Solar Magnetic Field, Line Of Sight, Magnetic Signatures, Radiation Distribution, Solar Limb
Scientific paper
Network magnetic fields are described as the dynamic product of the merging and cancelling of intranetwork fields, ephemeral regions, and the remnants of active regions. The similarities of these phenomena with solar magnetic features are pointed out. The intranetwork magnetic fields are characterized by the flow of successive fragments in approximately radial patterns away from their apparent source sites.
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