The relationship between coronal streamers and CMEs.

Details The relationship between coronal streamers and CMEs. The relationship between coronal streamers and CMEs.

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ppmto..18..135d&link_type=abstract

Publ. Purple Mt. Obs., Vol. 18, No. 2, p. 135 - 138

Physics

Solar Corona: Mass Ejection, Solar Corona: Streamers

Scientific paper

The variation of the polarization brightness of coronal streamer in Carrington Rotations 1591 - 1592 is investigated. The distribution of the polarization brightness along streamer belts is inhomogeneous; the degree of the inhomogeneity is 10% - 50%. In the absence of coronal mass ejection (CME) influence, the distribution of coronal streamers along the streamer belts can persist stable during nearly two Carrington Rotations. The rise velocity of the top of the cusp region in a coronal streamer may be more than 2 km/s, if the longitude angular size is more than 27° associated with a CME occurrence.

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