The X-UV spectrum of thin plasmas

Statistics – Computation

Scientific paper

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Computational Astrophysics, Cosmic Plasma, Far Ultraviolet Radiation, High Temperature Plasmas, Abundance, Emission Spectra, Ion Production Rates, Optical Thickness, Solar Corona

Scientific paper

The spectrum of the radiation emitted by a hot (10,000-100 million K)
and optically thin plasma is computed in the spectral range 1-2000 A.
Comparison is made with previous computations and differences are
discussed.

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