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000 | 05048naa a2201009 4500 | |
001 | oai:gup.ub.gu.se/160468 | |
003 | SwePub | |
008 | 240528s2012 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:ltu-12146 | |
024 | 7 | a https://gup.ub.gu.se/publication/1604682 URI |
024 | 7 | a https://doi.org/10.1016/j.jqsrt.2011.11.0042 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-121462 URI |
040 | a (SwePub)gud (SwePub)ltu | |
041 | a eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Richard, C.u Harvard-Smithsonian Center for Astrophysics4 aut |
245 | 1 0 | a New section of the HITRAN database: Collision-induced absorption (CIA) |
264 | 1 | b Elsevier BV,c 2012 |
500 | a Upprättat; 2012; 20141017 (maggus) | |
520 | a This paper describes the addition of Collision-Induced Absorption (CIA) into the HITRAN compilation. The data from different experimental and theoretical sources have been cast into a consistent format and formalism. The implementation of these new spectral data into the HITRAN database is invaluable for modeling and interpreting spectra of telluric and other planetary atmospheres as well as stellar atmospheres. In this implementation for HITRAN, CIAs of N-2, H-2, O-2, CO2, and CH4 due to various collisionally interacting atoms or molecules are presented. Some CIA spectra are given over an extended range of frequencies, including several H-2 overtone bands that are dipole-forbidden in the non-interacting molecules. Temperatures from tens to thousands of Kelvin are considered, as required, for example, in astrophysical analyses of objects, including cool white dwarfs, brown dwarfs. M dwarfs, cool main sequence stars, solar and extra-solar planets, and the formation of so-called first stars. (C) 2011 Elsevier Ltd. All rights reserved. | |
650 | 7 | a NATURVETENSKAPx Kemi0 (SwePub)1042 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Chemical Sciences0 (SwePub)1042 hsv//eng |
650 | 7 | a NATURVETENSKAPx Fysikx Annan fysik0 (SwePub)103992 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Other Physics Topics0 (SwePub)103992 hsv//eng |
653 | a Collision-induced absorption | |
653 | a HITRAN | |
653 | a Atmospheric absorption | |
653 | a Interacting molecular pairs | |
653 | a cool white-dwarfs | |
653 | a molecular spectroscopic database | |
653 | a infrared-absorption | |
653 | a model atmospheres | |
653 | a titans atmosphere | |
653 | a earths | |
653 | a atmosphere | |
653 | a low-temperatures | |
653 | a brown dwarfs | |
653 | a 1st stars | |
653 | a a-band | |
653 | a RS | |
653 | a UMR 7583 | |
653 | a F-94010 Creteil | |
653 | a France. | |
653 | a [Hermans | |
653 | a C.] Belgian Inst Space Aeron | |
653 | a B-1180 Brussels | |
653 | a Belgium. | |
653 | a [Lafferty | |
653 | a W. J.] NIST | |
653 | a Opt Technol Div | |
653 | a Gaithersburg | |
653 | a MD 20899 USA. | |
653 | a [Orton | |
653 | a G. S.] CALTECH | |
653 | a Jet Prop Lab | |
653 | a Pasadena | |
653 | a CA 91109 USA. | |
653 | a [Smith | |
653 | a K. M.] RAL Space | |
653 | a Rutherford Appleton Lab | |
653 | a Didcot | |
653 | a Oxon | |
653 | a England. | |
653 | a kellar ar | |
653 | a 1972 | |
653 | a canadian journal of physics | |
653 | a v50 | |
653 | a p1 | |
653 | a Tillämpad fysik | |
700 | 1 | a Gordon, I. E.u Harvard-Smithsonian Center for Astrophysics4 aut |
700 | 1 | a Rothman, L. S.u Harvard-Smithsonian Center for Astrophysics4 aut |
700 | 1 | a Abel, M.u University of Texas, Physics Department4 aut |
700 | 1 | a Frommhold, L.u University of Texas, Physics Department4 aut |
700 | 1 | a Gustafsson, Magnus,d 1969u Gothenburg University,Göteborgs universitet,Institutionen för kemi och molekylärbiologi,Department of Chemistry and Molecular Biology,Department of Chemistry and Molecular Biology, University of Gothenburg4 aut0 (Swepub:ltu)maggus |
700 | 1 | a Hartmann, J. M.u Université Paris Est Créteil, CNRS4 aut |
700 | 1 | a Hermans, C.u Belgian Institute for Space Aeronomy, Brussels4 aut |
700 | 1 | a Lafferty, W. J.u National Institute of Standards and Technology, Gaithersburg, USA4 aut |
700 | 1 | a Orton, G. S.u Jet Propulsion Laboratory, California Institute of Technology, Pasadena4 aut |
700 | 1 | a Smith, K. M.u Rutherford Appleton Laboratory, Oxfordshire4 aut |
700 | 1 | a Tran, H.u Université Paris Est Créteil, CNRS4 aut |
710 | 2 | a Harvard-Smithsonian Center for Astrophysicsb University of Texas, Physics Department4 org |
773 | 0 | t Journal of Quantitative Spectroscopy & Radiative Transferd : Elsevier BVg 113:11, s. 1276-1285q 113:11<1276-1285x 0022-4073x 1879-1352 |
856 | 4 8 | u https://gup.ub.gu.se/publication/160468 |
856 | 4 8 | u https://doi.org/10.1016/j.jqsrt.2011.11.004 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-12146 |
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