Planetary Shadow-Aware Distance Sampling

dc.contributor.authorBreyer, Carlen_US
dc.contributor.authorZirr, Tobiasen_US
dc.contributor.editorGhosh, Abhijeeten_US
dc.contributor.editorWei, Li-Yien_US
dc.date.accessioned2022-07-01T15:37:56Z
dc.date.available2022-07-01T15:37:56Z
dc.date.issued2022
dc.description.abstractDusk and dawn scenes have been difficult for brute force path tracers to handle. We identify that a major source of the inefficiency in explicitly path tracing the atmosphere in such conditions stems from wasting samples on the denser lower parts of atmosphere that get shadowed by the planet before the upper, thinner parts when the star sets below the horizon. We present a technique that overcomes this issue by sampling the star only from the unshadowed segments along rays based on boundaries found by intersecting a cylinder fit to the planet's shadow. We also sample the transmittance by mapping the distances of the boundaries to opacities and sampling the visible segments uniformly in opacity space. Our technique can achieve similar quality compared to brute-force path tracing at around a 60th of the time in such conditions.en_US
dc.description.sectionheadersSampling
dc.description.seriesinformationEurographics Symposium on Rendering
dc.identifier.doi10.2312/sr.20221152
dc.identifier.isbn978-3-03868-187-8
dc.identifier.issn1727-3463
dc.identifier.pages23-28
dc.identifier.pages6 pages
dc.identifier.urihttps://doi.org/10.2312/sr.20221152
dc.identifier.urihttps://diglib.eg.org:443/handle/10.2312/sr20221152
dc.publisherThe Eurographics Associationen_US
dc.rightsAttribution 4.0 International License
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.subjectCCS Concepts: Computing methodologies --> Ray tracing; Visibility
dc.subjectComputing methodologies
dc.subjectRay tracing
dc.subjectVisibility
dc.titlePlanetary Shadow-Aware Distance Samplingen_US
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