Chromospheric Filament Network and Coronal Streamers

Details Chromospheric Filament Network and Coronal Streamers Chromospheric Filament Network and Coronal Streamers

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..368..355p&link_type=abstract

The Physics of Chromospheric Plasmas ASP Conference Series, Vol. 368, Proceedings of the conference held 9-13 October, 2006 at t

Physics

Scientific paper

We searched the anchoring distribution of coronal streamers as recorded by the LASCO C2 and C3 instruments of SOHO, using synoptic maps of filaments. Synoptic maps of the inner corona based on measurements of the intensity of the coronal emission line at 530.3 nm and synoptic maps of solar magnetic fields have been used as well. We suggest that the determinative condition for the formation of a stable streamer is a strong magnetic field.

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