2016
DOI: 10.1016/j.jms.2016.06.007
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The 2015 edition of the GEISA spectroscopic database

Abstract: The GEISA database (Gestion et Etude des Informations Spectroscopiques Atmosphériques: Management and Study of Atmospheric Spectroscopic Information) has been developed and maintained by the ARA/ABC(t) group at LMD since 1974. GEISA is constantly evolving, taking into account the best available spectroscopic data. This paper presents the 2015 release of GEISA (GEISA-2015), which updates the last edition of 2011 and celebrates the 40th anniversary of the database. Significant updates and additions have been imp… Show more

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Cited by 336 publications
(212 citation statements)
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“… Note . Most data can be found in the HITRAN (Massie & Hervig, ), GEISA (Jacquinet‐Husson et al, ), and ARIA (ARIA, ) spectral databases. OPAC = Optical Properties of Aerosols and Clouds; GADS = Global Aerosol Data Set; HITRAN = HIgh Resolution TRANsmission molecular absoption database; GEISA = Gestion et Etude des Informations Spectroscopiques Atmosphériques.…”
Section: Training the Nnmentioning
confidence: 99%
“… Note . Most data can be found in the HITRAN (Massie & Hervig, ), GEISA (Jacquinet‐Husson et al, ), and ARIA (ARIA, ) spectral databases. OPAC = Optical Properties of Aerosols and Clouds; GADS = Global Aerosol Data Set; HITRAN = HIgh Resolution TRANsmission molecular absoption database; GEISA = Gestion et Etude des Informations Spectroscopiques Atmosphériques.…”
Section: Training the Nnmentioning
confidence: 99%
“…Some of this information is provided by spectroscopic databases [4,5] , but there are large gaps in the coverage. Al Derzi et al [6] give a comprehensive review of high resolution spectroscopic data recorded and analysed up to 2014.…”
Section: Introductionmentioning
confidence: 99%
“…The rather strong m 6 band of CH 3 I, located at 892.916 cm À1 , which coincides with the 11 lm window of transparency in the atmosphere [2][3][4], could therefore be a good candidate for such detection. However, no spectroscopic parameters exist for this molecule in the common access spectroscopic databases HITRAN [https://www.cfa.harvard.edu/hitran/] [5] or GEISA [http://ether.ipsl.jussieu.fr/etherTypo/?id=950] [6]. This work, which deals with line positions, is the very first contribution to fill this gap.…”
Section: Introductionmentioning
confidence: 99%