Matter flow velocities in the active region emission loop observed in the solar H-alpha line

Details Matter flow velocities in the active region emission loop observed in the solar H-alpha line Matter flow velocities in the active region emission loop observed in the solar H-alpha line

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..253d&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, March 1989, p. 253-257. In Russian. In Russian.

Other

Emission Spectra, H Alpha Line, Solar Activity, Solar Spectra, Flow Velocity, Magnetic Dipoles

Scientific paper

The geometry of the emission loop in the active region is reconstructed and its true shape and size are determined. The loop was positioned almost vertically with respect to the solar surface and it tilted in its own plane. The loop matter rose from the solar surface along one leg with velocities of 105-35 km/s and it descended along the other leg with velocities of 14-65 km/s. The shape of the loop corresponded well with the magnetic dipole field line.

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