The evolution of longitudinal magnetic neutral line and chromospheric matter flow in solar active region.

Details The evolution of longitudinal magnetic neutral line and chromospheric matter flow in solar active region. The evolution of longitudinal magnetic neutral line and chromospheric matter flow in solar active region.

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pbeio..14...68z&link_type=abstract

Publications of the Beijing Astronomical Observatory, No. 14, p. 68 - 77

Astronomy and Astrophysics

Astronomy

Solar Active Regions: Solar Photosphere, Solar Active Regions: Chromospheres, Solar Active Regions: Magnetic Fields

Scientific paper

The authors discuss the photospheric and chromospheric vector magnetic
fields and matter flows in the active regions, especially the relations
between the matter flows and the evolution of the magnetic fields near
the area of the longitudinal magnetic neutral line.

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