Plasma Flows in Coronal Streamers-Numerical Simulation

Details Plasma Flows in Coronal Streamers-Numerical Simulation Plasma Flows in Coronal Streamers-Numerical Simulation

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..934..129d&link_type=abstract

FLOWS, BOUNDARIES, INTERACTIONS: Flows, Boundaries, and Interaction Workshop. AIP Conference Proceedings, Volume 934, pp. 129-1

Computer Science

Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation, Particle Emission, Solar Wind, Electric And Magnetic Fields, Solar Magnetism

Scientific paper

Coronal streamers are very interesting, long lived, features of solar corona. They are linked to prominences, CMEs and also to slow solar wind. The have different shape and behavior. We present a numerical simulation of a coronal streamer computed on five solar radii. Vertical motions in the streamer, both ascending and descending, are revealed during the streamer evolution, as well as eddy flows.

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