On the relation between large scale solar magnetic fields and filament positions

Details On the relation between large scale solar magnetic fields and filament positions On the relation between large scale solar magnetic fields and filament positions

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983basi...11..327s&link_type=abstract

Astronomical Society of India, Bulletin, vol. 11, Dec. 1983, p. 327-336.

Astronomy and Astrophysics

Astronomy

3

Filaments, H Alpha Line, Position (Location), Solar Magnetic Field, Solar Prominences, Graphs (Charts), Magnetic Field Configurations, Magnetic Signatures, Solar Rotation

Scientific paper

Interrelationships of filament positions and large scale solar magnetic
field structures are examined here. The broad neutral bands seem to be
suitable locations for the formation and development of filaments.
Filaments generally break into fragments as soon as narrow neutral bands
are formed.

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