Reconstruction of the geometry and matter motion velocities in an emission loop observed on the solar disk in the Hα line.

Details Reconstruction of the geometry and matter motion velocities in an emission loop observed on the solar disk in the Hα line. Reconstruction of the geometry and matter motion velocities in an emission loop observed on the solar disk in the Hα line.

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989bsold..11..110d&link_type=abstract

Byulletin Solnechnye Dannye Akademie Nauk USSR, No. 1989/1011 p. 110 - 114

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Solar Coronal Loops: Solar Active Regions

Scientific paper

An active region emission loop has been reconstructed, its true form and size have been determined. The loop proved to be almost vertical to the solar surface and only slightly tilted in the own plane. The loop matter has been found to rise from the solar surface along one leg with velocities 35 - 105 m/s and to descend along the other leg with velocities 14 - 65 km/s. The loop has been shown to have a close correspondence to the magnetic dipole field line.

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