Spectral Constraints on the Heating of CME Plasmas

Details Spectral Constraints on the Heating of CME Plasmas Spectral Constraints on the Heating of CME Plasmas

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufmsh44a..04r&link_type=abstract

American Geophysical Union, Fall Meeting 2005, abstract #SH44A-04

Physics

7513 Coronal Mass Ejections (2101), 7526 Magnetic Reconnection (2723, 7835), 7531 Prominence Eruptions, 7549 Ultraviolet Emissions

Scientific paper

The leading edge of a fast CME is heated by a shock wave. The bulk CME plasma is not shocked, but it is heated by some as yet poorly constrained mechanism. We discuss recent results for the amounts of heating and the partition of the energy among different particle species both for shocks and for the plasma in the CME interior. We will also discuss the powerful diagnostics available for future spectroscopic missions.

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