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Paper: Challenges in the Solution of the Transfer Equation in Multi-D Hydrodynamical Model Atmospheres for Cool Stars
Volume: 288, Stellar Atmosphere Modeling
Page: 537
Authors: Ludwig, H.-G.
Abstract: 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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