The Influence Of Helium Ions And Heating On Coronal Streamer Structure

Details The Influence Of Helium Ions And Heating On Coronal Streamer Structure The Influence Of Helium Ions And Heating On Coronal Streamer Structure

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.3001o&link_type=abstract

American Astronomical Society Meeting 210, #30.01; Bulletin of the American Astronomical Society, Vol. 39, p.142

Astronomy and Astrophysics

Astronomy

Scientific paper

The magnetic and compositional structure and dynamics of a coronal streamer is investigated using thermally conductive multi-fluid model. The variation of proton density, and He I/He II abundances is studied as a function of latitude and height. The effects of various heating rates, and heating profiles on the formation, and the compositional structure of streamers are studied. The dependence of the acceleration profile of the multi-component slow solar wind, as well as the properties of the differential ion outflow on the heat input is investigated numerically and compared to observations.

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