A note on improved computations of solar prominences: 2D radiative models.

Details A note on improved computations of solar prominences: 2D radiative models. A note on improved computations of solar prominences: 2D radiative models.

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...311..708p&link_type=abstract

Astronomy and Astrophysics, v.311, p.708-709

Astronomy and Astrophysics

Astrophysics

10

Radiative Transfer, Sun: Prominences

Scientific paper

We report on improved computations concerning two-dimensional (2D) radiative modelling of solar prominences. This report mainly concerns a more correct definition of the bound-free radiative rates (incident radiation and dilution factor). As a consequence, the difference (at a given height) between the Hα line integrated intensity computed respectively in 1D and 2D geometries is found to be less important than what was previously presented (Paletou 1995).

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