The role of radiative losses in the late evolution of pulse-heated coronal loops/strands

Author： Reale F.   Landi E.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|543|issue|A90-A90

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.543, Iss.issue, 2012-07, pp. : A90-A90

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Abstract

Context. Radiative losses from optically thin plasma are an important ingredient in modeling confined plasma in the solar corona. Spectral models are continuously updated to include the emission from more spectral lines, with significant effects on radiative losses, especially around 1 MK.

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