On boundaries among magnetic structures at the sun

Details On boundaries among magnetic structures at the sun On boundaries among magnetic structures at the sun

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990an....311..397i&link_type=abstract

Astronomische Nachrichten (ISSN 0004-6337), vol. 311, no. 6, 1990, p. 397, 398.

Astronomy and Astrophysics

Astronomy

Magnetic Field Configurations, Solar Atmosphere, Solar Flares, Solar Magnetic Field, Chromosphere, Solar Corona, Sunspots

Scientific paper

Results of an analysis of published observational data on large complex active regions (CARs) on the sun are briefly discussed. Boundaries detected in the lower region of the solar atmosphere are shown to reveal the separation of independently developing magnetic structures, which may interact to produce eruption effects such as flares, reconnection, and flux-tube cancelling, as proposed by Linke and Bachmann (1989). The characteristics of these boundaries are illustrated with diagrams based on CAR data for June-July 1982, July-August 1983, and October 1979.

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