Solar atmospheric responses to magnetic flux eruptions. I. A mechanism for coronal mass ejections

Details Solar atmospheric responses to magnetic flux eruptions. I. A mechanism for coronal mass ejections Solar atmospheric responses to magnetic flux eruptions. I. A mechanism for coronal mass ejections

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991cha%26a..15..284h&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 15, Issue 3, p. 284-291.

Astronomy and Astrophysics

Astrophysics

Sun-Magnetic Field-Coral Mass Ejection

Scientific paper

He carried out a numerical simulation of atmospheric responses to magnetic flux eruptions from the base of a helmet streamer. The results show that the material originally contained in the streamer is compressed and lifted upward by the erupting magnetic field, forming a high density bright loop. At the same time, fast magnetosonic waves appear in front of the loop and a low density dark region, below it. These results suggest that magnetic flux eruption is probably an important triggering mechanism of loop-like coronal mass ejection.

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