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L773:1077 2626 OR L773:1941 0506 OR L773:2160 9306
 

Sökning: L773:1077 2626 OR L773:1941 0506 OR L773:2160 9306 > Interactive Visuali...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00004104naa a2200373 4500
001oai:DiVA.org:liu-175102
003SwePub
008210421s2021 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:liu:diva-1751022 URI
024a https://doi.org/10.1109/TVCG.2020.30303332 DOI
040 a (SwePub)liu
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Costa, Jonathasu NYU, NY 10003 USA4 aut
2451 0a Interactive Visualization of Atmospheric Effects for Celestial Bodies
264 1b IEEE COMPUTER SOC,c 2021
338 a electronic2 rdacarrier
500 a Funding Agencies|NASANational Aeronautics & Space Administration (NASA) [NNX16AB93A]; VRSwedish Research Council [2015-05462]; Swedish e-Science Research Centre; NSFNational Science Foundation (NSF) [CNS-1229185, CCF-1533564, CNS-15447.53, CNS-1626098, CNS-1730396, CNS-1828576]; Knut Alice Wallenberg Foundation through the WISDOME project
520 a We present an atmospheric model tailored for the interactive visualization of planetary surfaces. As the exploration of the solar system is progressing with increasingly accurate missions and instruments, the faithful visualization of planetary environments is gaining increasing interest in space research, mission planning, and science communication and education. Atmospheric effects are crucial in data analysis and to provide contextual information for planetary data. Our model correctly accounts for the non-linear path of the light inside the atmosphere (in Earths case), the light absorption effects by molecules and dust particles, such as the ozone layer and the Martian dust, and a wavelength-dependent phase function for Mie scattering. The mode focuses on interactivity, versatility, and customization, and a comprehensive set of interactive controls make it possible to adapt its appearance dynamically. We demonstrate our results using Earth and Mars as examples. However, it can be readily adapted for the exploration of other atmospheres found on, for example, of exoplanets. For Earths atmosphere, we visually compare our results with pictures taken from the International Space Station and against the CIE clear sky model. The Martian atmosphere is reproduced based on available scientific data, feedback from domain experts, and is compared to images taken by the Curiosity rover. The work presented here has been implemented in the OpenSpace system, which enables interactive parameter setting and real-time feedback visualization targeting presentations in a wide range of environments, from immersive dome theaters to virtual reality headsets.
650 7a NATURVETENSKAPx Data- och informationsvetenskapx Annan data- och informationsvetenskap0 (SwePub)102992 hsv//swe
650 7a NATURAL SCIENCESx Computer and Information Sciencesx Other Computer and Information Science0 (SwePub)102992 hsv//eng
653 a Physical & Environmental Sciences; Engineering; Mathematics; Computer Graphics Techniques
700a Bock, Alexanderu Linköpings universitet,Medie- och Informationsteknik,Tekniska fakulteten,Univ Utah, UT 84112 USA4 aut0 (Swepub:liu)alebo68
700a Emmart, Carteru Amer Museum Nat Hist, NY 10024 USA4 aut
700a Hansen, Charlesu Univ Utah, UT 84112 USA4 aut
700a Ynnerman, Andersu Linköpings universitet,Medie- och Informationsteknik,Tekniska fakulteten,Centrum för medicinsk bildvetenskap och visualisering, CMIV,Univ Utah, UT 84112 USA4 aut0 (Swepub:liu)andyn27
700a Silva, Claudiou NYU, NY 10003 USA4 aut
710a NYU, NY 10003 USAb Medie- och Informationsteknik4 org
773t IEEE Transactions on Visualization and Computer Graphicsd : IEEE COMPUTER SOCg 27:2, s. 785-795q 27:2<785-795x 1077-2626x 1941-0506
856u https://liu.diva-portal.org/smash/get/diva2:1546184/FULLTEXT01.pdfx primaryx Raw objecty fulltext:postprint
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:liu:diva-175102
8564 8u https://doi.org/10.1109/TVCG.2020.3030333

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