The motion of solar coronal loop transients (II).

Details The motion of solar coronal loop transients (II). The motion of solar coronal loop transients (II).

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983acaps...3...26l&link_type=abstract

Acta Astrophys. Sin., Vol. 3, No. 1, p. 26 - 32

Astronomy and Astrophysics

Astrophysics

Magnetohydrodynamics:Solar Coronal Loops, Solar Coronal Loops:Magnetohydrodynamics, Solar Coronal Loops:Transients

Scientific paper

The mass ejection events of corona in the form of loop transients were discovered with white light photographs of the solar corona from Skylab. The author develops a magnetic flux tube model, in which a solar coronal loop is the tube of a magnetic force line. The forces driving the coronal loops are produced by a nonhomogeneous distribution of longitudinal magnetic fields in the magnetic flux tube. Numerical results of the model are compared with Skylab observations in the years 1973-1974.

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