Radiative losses of optically thin coronal plasmas

Details Radiative losses of optically thin coronal plasmas Radiative losses of optically thin coronal plasmas

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26a...347..401l&link_type=abstract

Astronomy and Astrophysics, v.347, p.401-408 (1999)

Astronomy and Astrophysics

Astrophysics

33

Plasmas, Radiation Mechanisms: Non-Thermal

Scientific paper

In the present work the total radiative losses and the total emissivity curve are calculated for an optically thin plasma using the Arcetri Spectral Code in the 10(4-10^8) temperature range. Checks have been made on the effects of changes in the parameters involved in the calculations, such as element abundances, ion fractions, electron density and transition probabilities on the resulting curves. Parametric fits are given for the resulting radiative losses curves and comparison is made with previous results.

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