X-ray emission spectra from ionizing plasmas

Details X-ray emission spectra from ionizing plasmas X-ray emission spectra from ionizing plasmas

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss..98..367m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 98, no. 2, Jan. 1984, p. 367-395.

Astronomy and Astrophysics

Astrophysics

120

Emission Spectra, Nonequilibrium Ionization, Nonequilibrium Plasmas, Plasma Spectra, X Ray Spectra, Eigenvalues, High Temperature Plasmas, Interstellar Matter, Ion Production Rates, Supernova Remnants

Scientific paper

Effects of non-equilibrium ionization on emission spectra are studied. Ionization rate equations are solved with the eigenvalue-method to avoid a numerical instability near the equilibrium and also to save time of computations. The author's scheme is valid for linear problems, and is applicable to solve closely coupled equations of time-dependent problems. As an example, he calculates emission spectra (1 - 160 Å) in the transient phase of ionization under interstellar conditions applicable to a shock-heated plasma. The results are useful for an analysis of the spectra from tenuous ionizing plasmas - such as supernova remnants.

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