The emergence of magnetic flux

Details The emergence of magnetic flux The emergence of magnetic flux

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph..100..397z&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 100, Oct. 1985, p. 397-414.

Physics

142

Magnetic Flux, Magnetic Signatures, Solar Magnetic Field, Solar Prominences, Sunspots, H Alpha Line, Heuristic Methods, Morphology

Scientific paper

The morphology and dynamics of emerging flux regions and arch filament systems are summarized, and detailed observations of a particular active region with emerging magnetic flux are discussed. The central part of the growing active region shows abnormal granulation and a weak magnetic field that is locally transverse. In the border zone, strong downward flows occur in the chromosphere and photosphere; small features with strong magnetic fields (faculae and pores) are formed here. Near the leading and following edge, sunspots are formed by the coalescence of such small magnetic elements. An heuristic model of an emergent magnetic loop-shaped bundle consisting of many flux tubes is used to interpret the observational data.

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