On the formation of active region prominences (H alpha filaments)

Details On the formation of active region prominences (H alpha filaments) On the formation of active region prominences (H alpha filaments)

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nascp2442...81r&link_type=abstract

In NASA. Goddard Space Flight Center Coronal and Prominence Plasmas p 81-87 (SEE N87-20871 13-92)

Physics

18

Chromosphere, Mass Flow, Solar Atmosphere, Solar Magnetic Field, Solar Physics, Solar Prominences, Sun, Sunspots, Evolution (Development), Polarity, Shear Flow

Scientific paper

Analysis of sequential Hα images of active region prominence
formation suggests that simple large-scale photospheric mass-motions may
play a key role in the formation of these long, thin, Hα
filaments.

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