Statistics – Computation
Scientific paper
Feb 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26as...82..229l&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 82, no. 2, Feb. 1990, p. 229-260.
Statistics
Computation
215
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.
Landini Massimo
Monsignori Fossi Brunella C.
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