Fe XVII Emission from Hot, Collisional Plasmas

Details Fe XVII Emission from Hot, Collisional Plasmas Fe XVII Emission from Hot, Collisional Plasmas

Jun 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..774..129b&link_type=abstract

X-RAY DIAGNOSTICS OF ASTROPHYSICAL PLASMAS: Theory, Experiment, and Observation. AIP Conference Proceedings, Volume 774, pp. 12

Astronomy and Astrophysics

Astrophysics

2

Plasma Collision Processes, Astrophysical Plasma, Electron Collisions, Magnetohydrodynamics And Plasmas, Electron Collisions

Scientific paper

The ratios of the Fe XVII 3s --> 2p transitions to that of the dominant 3d --> 2p transition measured in high-temperature tokamak plasmas are compared to solar and astrophysical observations. Good agreement is found, demonstrating that the collisional line formation processes active in opacity-free, low-density, high-temperature laboratory plasmas are a good description of those found in astrophysical plasmas.

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