Challenges in the Solution of the Transfer Equation in Multi-D Hydrodynamical Model Atmospheres for Cool Stars

Details Challenges in the Solution of the Transfer Equation in Multi-D Hydrodynamical Model Atmospheres for Cool Stars Challenges in the Solution of the Transfer Equation in Multi-D Hydrodynamical Model Atmospheres for Cool Stars

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aspc..288..537l&link_type=abstract

Stellar Atmosphere Modeling, ASP Conference Proceedings, Vol. 288. Abstracts from a conference held 8-12 April 2002 in Tuebingen

Astronomy and Astrophysics

Astronomy

1

Scientific paper

My talk is intended to stimulate discussions about methods in radiative transfer for hydrodynamical model atmospheres of late-type stars. I will present a number a number of inherent problems, show how they are presently tackled (if so), and ask for ideas for more efficient approaches. The transparencies of my talk can be found in
Transparencies (4.3Mb)

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