Observation of magnetic and velocity fields of enhanced network on the sun

Details Observation of magnetic and velocity fields of enhanced network on the sun Observation of magnetic and velocity fields of enhanced network on the sun

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989acasn..30..188l&link_type=abstract

(Acta Astronomica Sinica, vol. 30, no. 2, 1989, p. 188-193) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 14, March

Astronomy and Astrophysics

Astrophysics

Magnetic Flux, Solar Atmosphere, Solar Granulation, Solar Magnetic Field, Atmospheric Circulation, Fine Structure, Magnetic Signatures, Velocity Distribution

Scientific paper

The solar magnetic field telescope provides quasi-simultaneous, two-level, two-dimensional magnetic and velocity fields and a monochromatic image of the sun. By using this system, fine structures in the magnetic and velocity fields of enhanced networks on the solar disk were observed systematically. Good coincidence of the network boundaries and supergranules was found. Strong vertical flow was found in the boundaries of magnetic field networks. The combining of small networks into larger ones and the collapse of the small networks followed by the formation of the larger networks were also observed.

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