Radiative losses in solar and stellar coronae (Dudik+, 2011)

Details Radiative losses in solar and stellar coronae (Dudik+, 2011) Radiative losses in solar and stellar coronae (Dudik+, 2011)

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35299103d&link_type=abstract

VizieR On-line Data Catalog: J/A+A/529/A103. Originally published in: 2011A&A...529A.103D

Physics

Atomic Physics

Atomic Physics

Scientific paper

The radiative losses due to bound-bound and free-free transitions calculated for plasma with nonthermal {kappa}- and n-distributions of electron energies are presented. The radiative losses are calculated for the values of {kappa}=2, 3, 5, and 10 (rloss_k.dat) and n=1 (Maxwellian), 3, 5, and 11 (rloss_n.dat) as function of temperature (T) or pseudo-temperature (tau) for the assumed value of electron density ne=1016m-3. The ne*nH factor is not included in the calculations.
(2 data files).

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