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Paper: Chromospheric Filament Network and Coronal Streamers
Volume: 368, The Physics of Chromospheric Plasmas
Page: 355
Authors: Pinter, T.; Rybansky, M.; Dorotovic, I.
Abstract: 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 530.3nm 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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