Parallelization Strategies for ALI Radiative Transfer in Moving Media

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dc.creatorBaron, E.
dc.creatorHauschildt, P. H.
dc.creatorLowenthal, D.
dc.date2002-07-01
dc.date.accessioned2026-07-07T02:04:08Z
dc.date.available2026-07-07T02:04:08Z
dc.descriptionWe describe the method we have used to parallelize our spherically symmetric special relativistic short characteristics general radiative transfer code PHOENIX. We describe some possible parallelization strategies and show why they would be inefficient. We discuss the multiple parallelization strategy techniques that we have adopted. We briefly discuss generalizing these strategies to full 3-D (spatial) radiation transfer codes.
dc.description18 pages, 5 figures to appear in Stellar Atmospheric Modeling I. Hubeny, D. Mihalas, and K. Werner eds., (San Francisco: ASP)
dc.identifierhttps://arxiv.org/abs/astro-ph/0207043
dc.identifierhttp://arxiv.org/abs/astro-ph/0207043
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4633
dc.subjectAstrophysics
dc.titleParallelization Strategies for ALI Radiative Transfer in Moving Media
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