Please use this identifier to cite or link to this item: http://dx.doi.org/10.18419/opus-8033
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dc.contributor.authorErtl, Thomasde
dc.contributor.authorGeyer, Floriande
dc.contributor.authorHerold, Heinzde
dc.contributor.authorKraus, Utede
dc.contributor.authorNiemeier, Rolandde
dc.contributor.authorNollert, Hans-Peterde
dc.contributor.authorRebetzky, Andreasde
dc.contributor.authorRuder, Hannsde
dc.contributor.authorZeller, Gudrunde
dc.date.accessioned2012-09-05de
dc.date.accessioned2016-03-31T11:44:59Z-
dc.date.available2012-09-05de
dc.date.available2016-03-31T11:44:59Z-
dc.date.issued1989de
dc.identifier.other371577624de
dc.identifier.urihttp://nbn-resolving.de/urn:nbn:de:bsz:93-opus-76989de
dc.identifier.urihttp://elib.uni-stuttgart.de/handle/11682/8050-
dc.identifier.urihttp://dx.doi.org/10.18419/opus-8033-
dc.description.abstractThis paper reports on progress we have made in modelling cosmic X·ray sources on supercomputers. The results we present are meant to serve as an example for the fact that sophisticated visualization techniques play a crucial role in scientific computing. Among the graphical methods we demonstrate, raytracing in curved space-time and a physically motivated 3D-volume rendering algorithm might be of interest to the graphics community in general.en
dc.language.isoende
dc.rightsinfo:eu-repo/semantics/openAccessde
dc.subject.classificationComputersimulation , Röntgenpulsar , Magnetosphärede
dc.subject.ddc530de
dc.titleVisualization in astrophysicsen
dc.typeconferenceObjectde
dc.date.updated2012-09-25de
ubs.fakultaetFakultätsübergreifend / Sonstige Einrichtungde
ubs.institutSonstige Einrichtungde
ubs.opusid7698de
ubs.publikation.sourceEurographics (1989). Amsterdam : North-Holland Publ. Co., 1989. - ISBN 0-444-88013-5, S. 149-158de
ubs.publikation.typKonferenzbeitragde
Appears in Collections:15 Fakultätsübergreifend / Sonstige Einrichtung

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