The 2009 edition of the GEISA spectroscopic database

The updated 2009 edition of the spectroscopic database GEISA (Gestion et Etude des Informations Spectroscopiques Atmosphériques; Management and Study of Atmospheric Spectroscopic Information) is described in this paper. GEISA is a computer-accessible system comprising three independent sub-databases...

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Veröffentlicht in:Journal of quantitative spectroscopy & radiative transfer 2011-10, Vol.112 (15), p.2395-2445
Hauptverfasser: Jacquinet-Husson, N., Crepeau, L., Armante, R., Boutammine, C., Chédin, A., Scott, N.A., Crevoisier, C., Capelle, V., Boone, C., Poulet-Crovisier, N., Barbe, A., Campargue, A., Chris Benner, D., Benilan, Y., Bézard, B., Boudon, V., Brown, L.R., Coudert, L.H., Coustenis, A., Dana, V., Devi, V.M., Fally, S., Fayt, A., Flaud, J.-M., Goldman, A., Herman, M., Harris, G.J., Jacquemart, D., Jolly, A., Kleiner, I., Kleinböhl, A., Kwabia-Tchana, F., Lavrentieva, N., Lacome, N., Xu, Li-Hong, Lyulin, O.M., Mandin, J.-Y., Maki, A., Mikhailenko, S., Miller, C.E., Mishina, T., Moazzen-Ahmadi, N., Müller, H.S.P., Nikitin, A., Orphal, J., Perevalov, V., Perrin, A., Petkie, D.T., Predoi-Cross, A., Rinsland, C.P., Remedios, J.J., Rotger, M., Smith, M.A.H., Sung, K., Tashkun, S., Tennyson, J., Toth, R.A., Vandaele, A.-C., Vander Auwera, J.
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container_title Journal of quantitative spectroscopy & radiative transfer
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creator Jacquinet-Husson, N.
Crepeau, L.
Armante, R.
Boutammine, C.
Chédin, A.
Scott, N.A.
Crevoisier, C.
Capelle, V.
Boone, C.
Poulet-Crovisier, N.
Barbe, A.
Campargue, A.
Chris Benner, D.
Benilan, Y.
Bézard, B.
Boudon, V.
Brown, L.R.
Coudert, L.H.
Coustenis, A.
Dana, V.
Devi, V.M.
Fally, S.
Fayt, A.
Flaud, J.-M.
Goldman, A.
Herman, M.
Harris, G.J.
Jacquemart, D.
Jolly, A.
Kleiner, I.
Kleinböhl, A.
Kwabia-Tchana, F.
Lavrentieva, N.
Lacome, N.
Xu, Li-Hong
Lyulin, O.M.
Mandin, J.-Y.
Maki, A.
Mikhailenko, S.
Miller, C.E.
Mishina, T.
Moazzen-Ahmadi, N.
Müller, H.S.P.
Nikitin, A.
Orphal, J.
Perevalov, V.
Perrin, A.
Petkie, D.T.
Predoi-Cross, A.
Rinsland, C.P.
Remedios, J.J.
Rotger, M.
Smith, M.A.H.
Sung, K.
Tashkun, S.
Tennyson, J.
Toth, R.A.
Vandaele, A.-C.
Vander Auwera, J.
description The updated 2009 edition of the spectroscopic database GEISA (Gestion et Etude des Informations Spectroscopiques Atmosphériques; Management and Study of Atmospheric Spectroscopic Information) is described in this paper. GEISA is a computer-accessible system comprising three independent sub-databases devoted, respectively, to: line parameters, infrared and ultraviolet/visible absorption cross-sections, microphysical and optical properties of atmospheric aerosols. In this edition, 50 molecules are involved in the line parameters sub-database, including 111 isotopologues, for a total of 3,807,997 entries, in the spectral range from 10 −6 to 35,877.031 cm −1. The successful performances of the new generation of hyperspectral sounders depend ultimately on the accuracy to which the spectroscopic parameters of the optically active atmospheric gases are known, since they constitute an essential input to the forward radiative transfer models that are used to interpret their observations. Currently, GEISA is involved in activities related to the assessment of the capabilities of IASI (Infrared Atmospheric Sounding Interferometer; http://smsc.cnes.fr/IASI/index.htm) on board the METOP European satellite through the GEISA/IASI database derived from GEISA. Since the Metop-A ( http://www.eumetsat.int) launch (19 October 2006), GEISA is the reference spectroscopic database for the validation of the level-1 IASI data. Also, GEISA is involved in planetary research, i.e., modeling of Titan's atmosphere, in the comparison with observations performed by Voyager, or by ground-based telescopes, and by the instruments on board the Cassini–Huygens mission. GEISA, continuously developed and maintained at LMD (Laboratoire de Météorologie Dynamique, France) since 1976, is implemented on the IPSL/CNRS (France) “Ether” Products and Services Centre WEB site ( http://ether.ipsl.jussieu.fr), where all archived spectroscopic data can be handled through general and user friendly associated management software facilities. More than 350 researchers are registered for on line use of GEISA. ► Strong interaction with Earth's and planetary atmospheres remote sensing. ► Improvement of the quality of the direct and inverse planetary atmosphere modeling. ► Evident importance for Research in Climate and Environment.► Promotion and motivation for Research in Spectroscopy (theoretical and experimental).
doi_str_mv 10.1016/j.jqsrt.2011.06.004
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GEISA is a computer-accessible system comprising three independent sub-databases devoted, respectively, to: line parameters, infrared and ultraviolet/visible absorption cross-sections, microphysical and optical properties of atmospheric aerosols. In this edition, 50 molecules are involved in the line parameters sub-database, including 111 isotopologues, for a total of 3,807,997 entries, in the spectral range from 10 −6 to 35,877.031 cm −1. The successful performances of the new generation of hyperspectral sounders depend ultimately on the accuracy to which the spectroscopic parameters of the optically active atmospheric gases are known, since they constitute an essential input to the forward radiative transfer models that are used to interpret their observations. Currently, GEISA is involved in activities related to the assessment of the capabilities of IASI (Infrared Atmospheric Sounding Interferometer; http://smsc.cnes.fr/IASI/index.htm) on board the METOP European satellite through the GEISA/IASI database derived from GEISA. Since the Metop-A ( http://www.eumetsat.int) launch (19 October 2006), GEISA is the reference spectroscopic database for the validation of the level-1 IASI data. Also, GEISA is involved in planetary research, i.e., modeling of Titan's atmosphere, in the comparison with observations performed by Voyager, or by ground-based telescopes, and by the instruments on board the Cassini–Huygens mission. GEISA, continuously developed and maintained at LMD (Laboratoire de Météorologie Dynamique, France) since 1976, is implemented on the IPSL/CNRS (France) “Ether” Products and Services Centre WEB site ( http://ether.ipsl.jussieu.fr), where all archived spectroscopic data can be handled through general and user friendly associated management software facilities. More than 350 researchers are registered for on line use of GEISA. ► Strong interaction with Earth's and planetary atmospheres remote sensing. ► Improvement of the quality of the direct and inverse planetary atmosphere modeling. ► Evident importance for Research in Climate and Environment.► Promotion and motivation for Research in Spectroscopy (theoretical and experimental).</description><identifier>ISSN: 0022-4073</identifier><identifier>EISSN: 1879-1352</identifier><identifier>DOI: 10.1016/j.jqsrt.2011.06.004</identifier><language>eng</language><publisher>Elsevier Ltd</publisher><subject>Atmospheric absorption ; Atmospheric aerosols ; Atmospheric radiative transfer ; Atmospherics ; Chemical Sciences ; Cross-sections ; Earth's and planetary atmospheres ; GEISA ; Infrared ; Line parameters ; Management ; Mathematical models ; Molecular spectroscopy ; Optics ; or physical chemistry ; Physics ; Radiative transfer ; Spectroscopic analysis ; Spectroscopic database ; Spectroscopy ; Theoretical and</subject><ispartof>Journal of quantitative spectroscopy &amp; 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radiative transfer</title><description>The updated 2009 edition of the spectroscopic database GEISA (Gestion et Etude des Informations Spectroscopiques Atmosphériques; Management and Study of Atmospheric Spectroscopic Information) is described in this paper. GEISA is a computer-accessible system comprising three independent sub-databases devoted, respectively, to: line parameters, infrared and ultraviolet/visible absorption cross-sections, microphysical and optical properties of atmospheric aerosols. In this edition, 50 molecules are involved in the line parameters sub-database, including 111 isotopologues, for a total of 3,807,997 entries, in the spectral range from 10 −6 to 35,877.031 cm −1. The successful performances of the new generation of hyperspectral sounders depend ultimately on the accuracy to which the spectroscopic parameters of the optically active atmospheric gases are known, since they constitute an essential input to the forward radiative transfer models that are used to interpret their observations. Currently, GEISA is involved in activities related to the assessment of the capabilities of IASI (Infrared Atmospheric Sounding Interferometer; http://smsc.cnes.fr/IASI/index.htm) on board the METOP European satellite through the GEISA/IASI database derived from GEISA. Since the Metop-A ( http://www.eumetsat.int) launch (19 October 2006), GEISA is the reference spectroscopic database for the validation of the level-1 IASI data. Also, GEISA is involved in planetary research, i.e., modeling of Titan's atmosphere, in the comparison with observations performed by Voyager, or by ground-based telescopes, and by the instruments on board the Cassini–Huygens mission. GEISA, continuously developed and maintained at LMD (Laboratoire de Météorologie Dynamique, France) since 1976, is implemented on the IPSL/CNRS (France) “Ether” Products and Services Centre WEB site ( http://ether.ipsl.jussieu.fr), where all archived spectroscopic data can be handled through general and user friendly associated management software facilities. More than 350 researchers are registered for on line use of GEISA. ► Strong interaction with Earth's and planetary atmospheres remote sensing. ► Improvement of the quality of the direct and inverse planetary atmosphere modeling. ► Evident importance for Research in Climate and Environment.► Promotion and motivation for Research in Spectroscopy (theoretical and experimental).</description><subject>Atmospheric absorption</subject><subject>Atmospheric aerosols</subject><subject>Atmospheric radiative transfer</subject><subject>Atmospherics</subject><subject>Chemical Sciences</subject><subject>Cross-sections</subject><subject>Earth's and planetary atmospheres</subject><subject>GEISA</subject><subject>Infrared</subject><subject>Line parameters</subject><subject>Management</subject><subject>Mathematical models</subject><subject>Molecular spectroscopy</subject><subject>Optics</subject><subject>or physical chemistry</subject><subject>Physics</subject><subject>Radiative transfer</subject><subject>Spectroscopic analysis</subject><subject>Spectroscopic database</subject><subject>Spectroscopy</subject><subject>Theoretical and</subject><issn>0022-4073</issn><issn>1879-1352</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><recordid>eNp9kEFLwzAYhoMoOKe_wEtv6qH1-5I0bQ8expjbYODBeQ5ZmrKUbu2SbuC_N7PicacPXp734-Uh5BEhQUDxWif1wbs-oYCYgEgA-BUZYZ4VMbKUXpMRAKUxh4zdkjvvawBgDMWI8PXWRBSgiExpe9vuo7aK-pDNZ8vPSeQ7o3vXet12Vkel6tVGeXNPbirVePPwd8fk6322ni7i1cd8OZ2sYs2B9jGmFWO0EFCVqDFNNYpsoyhWWZqxItN5gSrNKFQCUkqBl0AzWplUKVXqjQE2Ji_D361qZOfsTrlv2SorF5OVPGcAgjLGixMG9mlgO9cejsb3cme9Nk2j9qY9epnnOWJOkQXy-SIZViJnAnMRUDagOjjwzlT_KxDk2bys5a95eTYvQYRFPLTehpYJbk7WOOm1NXsdDLugU5atvdj_AbJsiPM</recordid><startdate>20111001</startdate><enddate>20111001</enddate><creator>Jacquinet-Husson, N.</creator><creator>Crepeau, L.</creator><creator>Armante, R.</creator><creator>Boutammine, C.</creator><creator>Chédin, A.</creator><creator>Scott, N.A.</creator><creator>Crevoisier, C.</creator><creator>Capelle, V.</creator><creator>Boone, C.</creator><creator>Poulet-Crovisier, N.</creator><creator>Barbe, A.</creator><creator>Campargue, A.</creator><creator>Chris Benner, D.</creator><creator>Benilan, Y.</creator><creator>Bézard, B.</creator><creator>Boudon, V.</creator><creator>Brown, L.R.</creator><creator>Coudert, L.H.</creator><creator>Coustenis, A.</creator><creator>Dana, V.</creator><creator>Devi, V.M.</creator><creator>Fally, S.</creator><creator>Fayt, A.</creator><creator>Flaud, J.-M.</creator><creator>Goldman, A.</creator><creator>Herman, M.</creator><creator>Harris, G.J.</creator><creator>Jacquemart, D.</creator><creator>Jolly, A.</creator><creator>Kleiner, I.</creator><creator>Kleinböhl, A.</creator><creator>Kwabia-Tchana, F.</creator><creator>Lavrentieva, N.</creator><creator>Lacome, N.</creator><creator>Xu, Li-Hong</creator><creator>Lyulin, O.M.</creator><creator>Mandin, J.-Y.</creator><creator>Maki, A.</creator><creator>Mikhailenko, S.</creator><creator>Miller, C.E.</creator><creator>Mishina, T.</creator><creator>Moazzen-Ahmadi, N.</creator><creator>Müller, H.S.P.</creator><creator>Nikitin, A.</creator><creator>Orphal, J.</creator><creator>Perevalov, V.</creator><creator>Perrin, A.</creator><creator>Petkie, D.T.</creator><creator>Predoi-Cross, A.</creator><creator>Rinsland, C.P.</creator><creator>Remedios, J.J.</creator><creator>Rotger, M.</creator><creator>Smith, M.A.H.</creator><creator>Sung, K.</creator><creator>Tashkun, S.</creator><creator>Tennyson, J.</creator><creator>Toth, R.A.</creator><creator>Vandaele, A.-C.</creator><creator>Vander Auwera, J.</creator><general>Elsevier Ltd</general><general>Elsevier</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7SR</scope><scope>7U5</scope><scope>8BQ</scope><scope>8FD</scope><scope>JG9</scope><scope>L7M</scope><scope>7TG</scope><scope>KL.</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0001-9846-9816</orcidid><orcidid>https://orcid.org/0000-0002-8715-9764</orcidid><orcidid>https://orcid.org/0000-0001-7493-0719</orcidid><orcidid>https://orcid.org/0000-0002-4280-4096</orcidid><orcidid>https://orcid.org/0000-0002-5433-5661</orcidid><orcidid>https://orcid.org/0000-0003-3414-3491</orcidid><orcidid>https://orcid.org/0000-0001-5015-6538</orcidid><orcidid>https://orcid.org/0000-0002-9587-9884</orcidid><orcidid>https://orcid.org/0009-0004-9824-769X</orcidid></search><sort><creationdate>20111001</creationdate><title>The 2009 edition of the GEISA spectroscopic database</title><author>Jacquinet-Husson, N. ; Crepeau, L. ; Armante, R. ; Boutammine, C. ; Chédin, A. ; Scott, N.A. ; Crevoisier, C. ; Capelle, V. ; Boone, C. ; Poulet-Crovisier, N. ; Barbe, A. ; Campargue, A. ; Chris Benner, D. ; Benilan, Y. ; Bézard, B. ; Boudon, V. ; Brown, L.R. ; Coudert, L.H. ; Coustenis, A. ; Dana, V. ; Devi, V.M. ; Fally, S. ; Fayt, A. ; Flaud, J.-M. ; Goldman, A. ; Herman, M. ; Harris, G.J. ; Jacquemart, D. ; Jolly, A. ; Kleiner, I. ; Kleinböhl, A. ; Kwabia-Tchana, F. ; Lavrentieva, N. ; Lacome, N. ; Xu, Li-Hong ; Lyulin, O.M. ; Mandin, J.-Y. ; Maki, A. ; Mikhailenko, S. ; Miller, C.E. ; Mishina, T. ; Moazzen-Ahmadi, N. ; Müller, H.S.P. ; Nikitin, A. ; Orphal, J. ; Perevalov, V. ; Perrin, A. ; Petkie, D.T. ; Predoi-Cross, A. ; Rinsland, C.P. ; Remedios, J.J. ; Rotger, M. ; Smith, M.A.H. ; Sung, K. ; Tashkun, S. ; Tennyson, J. ; Toth, R.A. ; Vandaele, A.-C. ; Vander Auwera, J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c402t-15f332960fd1c155c167ba21f757397c891a5720f6052204d0272fe5aaadcbe03</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><topic>Atmospheric absorption</topic><topic>Atmospheric aerosols</topic><topic>Atmospheric radiative transfer</topic><topic>Atmospherics</topic><topic>Chemical Sciences</topic><topic>Cross-sections</topic><topic>Earth's and planetary atmospheres</topic><topic>GEISA</topic><topic>Infrared</topic><topic>Line parameters</topic><topic>Management</topic><topic>Mathematical models</topic><topic>Molecular spectroscopy</topic><topic>Optics</topic><topic>or physical chemistry</topic><topic>Physics</topic><topic>Radiative transfer</topic><topic>Spectroscopic analysis</topic><topic>Spectroscopic database</topic><topic>Spectroscopy</topic><topic>Theoretical and</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Jacquinet-Husson, N.</creatorcontrib><creatorcontrib>Crepeau, L.</creatorcontrib><creatorcontrib>Armante, R.</creatorcontrib><creatorcontrib>Boutammine, C.</creatorcontrib><creatorcontrib>Chédin, A.</creatorcontrib><creatorcontrib>Scott, N.A.</creatorcontrib><creatorcontrib>Crevoisier, C.</creatorcontrib><creatorcontrib>Capelle, V.</creatorcontrib><creatorcontrib>Boone, C.</creatorcontrib><creatorcontrib>Poulet-Crovisier, N.</creatorcontrib><creatorcontrib>Barbe, A.</creatorcontrib><creatorcontrib>Campargue, A.</creatorcontrib><creatorcontrib>Chris Benner, D.</creatorcontrib><creatorcontrib>Benilan, Y.</creatorcontrib><creatorcontrib>Bézard, B.</creatorcontrib><creatorcontrib>Boudon, V.</creatorcontrib><creatorcontrib>Brown, L.R.</creatorcontrib><creatorcontrib>Coudert, L.H.</creatorcontrib><creatorcontrib>Coustenis, A.</creatorcontrib><creatorcontrib>Dana, V.</creatorcontrib><creatorcontrib>Devi, V.M.</creatorcontrib><creatorcontrib>Fally, S.</creatorcontrib><creatorcontrib>Fayt, A.</creatorcontrib><creatorcontrib>Flaud, J.-M.</creatorcontrib><creatorcontrib>Goldman, A.</creatorcontrib><creatorcontrib>Herman, M.</creatorcontrib><creatorcontrib>Harris, G.J.</creatorcontrib><creatorcontrib>Jacquemart, D.</creatorcontrib><creatorcontrib>Jolly, A.</creatorcontrib><creatorcontrib>Kleiner, I.</creatorcontrib><creatorcontrib>Kleinböhl, A.</creatorcontrib><creatorcontrib>Kwabia-Tchana, F.</creatorcontrib><creatorcontrib>Lavrentieva, N.</creatorcontrib><creatorcontrib>Lacome, N.</creatorcontrib><creatorcontrib>Xu, Li-Hong</creatorcontrib><creatorcontrib>Lyulin, O.M.</creatorcontrib><creatorcontrib>Mandin, J.-Y.</creatorcontrib><creatorcontrib>Maki, A.</creatorcontrib><creatorcontrib>Mikhailenko, S.</creatorcontrib><creatorcontrib>Miller, C.E.</creatorcontrib><creatorcontrib>Mishina, T.</creatorcontrib><creatorcontrib>Moazzen-Ahmadi, N.</creatorcontrib><creatorcontrib>Müller, H.S.P.</creatorcontrib><creatorcontrib>Nikitin, A.</creatorcontrib><creatorcontrib>Orphal, J.</creatorcontrib><creatorcontrib>Perevalov, V.</creatorcontrib><creatorcontrib>Perrin, A.</creatorcontrib><creatorcontrib>Petkie, D.T.</creatorcontrib><creatorcontrib>Predoi-Cross, A.</creatorcontrib><creatorcontrib>Rinsland, C.P.</creatorcontrib><creatorcontrib>Remedios, J.J.</creatorcontrib><creatorcontrib>Rotger, M.</creatorcontrib><creatorcontrib>Smith, M.A.H.</creatorcontrib><creatorcontrib>Sung, K.</creatorcontrib><creatorcontrib>Tashkun, S.</creatorcontrib><creatorcontrib>Tennyson, J.</creatorcontrib><creatorcontrib>Toth, R.A.</creatorcontrib><creatorcontrib>Vandaele, A.-C.</creatorcontrib><creatorcontrib>Vander Auwera, J.</creatorcontrib><collection>CrossRef</collection><collection>Engineered Materials Abstracts</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>METADEX</collection><collection>Technology Research Database</collection><collection>Materials Research Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Meteorological &amp; 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radiative transfer</jtitle><date>2011-10-01</date><risdate>2011</risdate><volume>112</volume><issue>15</issue><spage>2395</spage><epage>2445</epage><pages>2395-2445</pages><issn>0022-4073</issn><eissn>1879-1352</eissn><abstract>The updated 2009 edition of the spectroscopic database GEISA (Gestion et Etude des Informations Spectroscopiques Atmosphériques; Management and Study of Atmospheric Spectroscopic Information) is described in this paper. GEISA is a computer-accessible system comprising three independent sub-databases devoted, respectively, to: line parameters, infrared and ultraviolet/visible absorption cross-sections, microphysical and optical properties of atmospheric aerosols. In this edition, 50 molecules are involved in the line parameters sub-database, including 111 isotopologues, for a total of 3,807,997 entries, in the spectral range from 10 −6 to 35,877.031 cm −1. The successful performances of the new generation of hyperspectral sounders depend ultimately on the accuracy to which the spectroscopic parameters of the optically active atmospheric gases are known, since they constitute an essential input to the forward radiative transfer models that are used to interpret their observations. Currently, GEISA is involved in activities related to the assessment of the capabilities of IASI (Infrared Atmospheric Sounding Interferometer; http://smsc.cnes.fr/IASI/index.htm) on board the METOP European satellite through the GEISA/IASI database derived from GEISA. Since the Metop-A ( http://www.eumetsat.int) launch (19 October 2006), GEISA is the reference spectroscopic database for the validation of the level-1 IASI data. Also, GEISA is involved in planetary research, i.e., modeling of Titan's atmosphere, in the comparison with observations performed by Voyager, or by ground-based telescopes, and by the instruments on board the Cassini–Huygens mission. GEISA, continuously developed and maintained at LMD (Laboratoire de Météorologie Dynamique, France) since 1976, is implemented on the IPSL/CNRS (France) “Ether” Products and Services Centre WEB site ( http://ether.ipsl.jussieu.fr), where all archived spectroscopic data can be handled through general and user friendly associated management software facilities. More than 350 researchers are registered for on line use of GEISA. ► Strong interaction with Earth's and planetary atmospheres remote sensing. ► Improvement of the quality of the direct and inverse planetary atmosphere modeling. ► Evident importance for Research in Climate and Environment.► Promotion and motivation for Research in Spectroscopy (theoretical and experimental).</abstract><pub>Elsevier Ltd</pub><doi>10.1016/j.jqsrt.2011.06.004</doi><tpages>51</tpages><orcidid>https://orcid.org/0000-0001-9846-9816</orcidid><orcidid>https://orcid.org/0000-0002-8715-9764</orcidid><orcidid>https://orcid.org/0000-0001-7493-0719</orcidid><orcidid>https://orcid.org/0000-0002-4280-4096</orcidid><orcidid>https://orcid.org/0000-0002-5433-5661</orcidid><orcidid>https://orcid.org/0000-0003-3414-3491</orcidid><orcidid>https://orcid.org/0000-0001-5015-6538</orcidid><orcidid>https://orcid.org/0000-0002-9587-9884</orcidid><orcidid>https://orcid.org/0009-0004-9824-769X</orcidid></addata></record>
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ispartof Journal of quantitative spectroscopy & radiative transfer, 2011-10, Vol.112 (15), p.2395-2445
issn 0022-4073
1879-1352
language eng
recordid cdi_hal_primary_oai_HAL_hal_00623349v1
source Elsevier ScienceDirect Journals
subjects Atmospheric absorption
Atmospheric aerosols
Atmospheric radiative transfer
Atmospherics
Chemical Sciences
Cross-sections
Earth's and planetary atmospheres
GEISA
Infrared
Line parameters
Management
Mathematical models
Molecular spectroscopy
Optics
or physical chemistry
Physics
Radiative transfer
Spectroscopic analysis
Spectroscopic database
Spectroscopy
Theoretical and
title The 2009 edition of the GEISA spectroscopic database
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