Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000adnx.conf..127f&link_type=abstract
Atomic Data Needs for X-ray Astronomy, p. 127
Astronomy and Astrophysics
Astrophysics
2
Extreme Ultraviolet Radiation, Plasmas (Physics), Tokamak Devices, X Ray Astronomy, X Ray Spectra, Astrophysics, Iron, Neon, Calcium, Spectral Resolution, Energy Levels, Computerized Simulation
Scientific paper
This paper presents the measured x-ray and Extreme Ultraviolet (XUV) spectra of three astrophysically abundant elements (Fe, Ca and Ne) from three different tokamak plasmas. In every case, each spectrum touches on an issue of atomic physics that is important for simulation codes to be used in the analysis of high spectral resolution data from current and future x-ray telescopes. The utility of the tokamak as a laboratory test bed for astrophysical data is demonstrated. Simple models generated with the HULLAC suite of codes demonstrate how the atomic physics issues studied can affect the interpretation of astrophysical data.
Finkenthal Michael
Fournier Kevin B.
Leigheb M.
Mattioli M. M.
May Michael J.
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