Following the Trail of Heavy Ions through the Solar Corona and into the Solar Wind

Details Following the Trail of Heavy Ions through the Solar Corona and into the Solar Wind Following the Trail of Heavy Ions through the Solar Corona and into the Solar Wind

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...21011103h&link_type=abstract

American Astronomical Society Meeting 210, #111.03; Bulletin of the American Astronomical Society, Vol. 39, p.235

Astronomy and Astrophysics

Astronomy

Scientific paper

Spectroscopy of the solar corona continues to play a key role for exploring the physical processes that define the properties of this optically thin plasma and control the acceleration of the solar wind. These processes determine the range of observed species temperatures, flow speeds and densities in different magnetic structures in the corona. This presentation will focus on the diagnostic power of spectroscopic observations of different ion species for exploring these physical processes. Particular emphasis will be placed on the non-negligible role played by heavy ions. A direct example for their behavior will be highlighted using results from the recent eclipse observations of 29 March 2006.

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