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dc.creatorCamy-Peyret, C.en_US
dc.date.accessioned2006-06-15T18:56:36Z
dc.date.available2006-06-15T18:56:36Z
dc.date.issued1993en_US
dc.identifier1993-WA-2en_US
dc.identifier.urihttp://hdl.handle.net/1811/18680
dc.descriptionAuthor Institution: Laboratoire de Physique mol\'{e}culaire et Applications, CNRS, Universit\'{e} P. et N. Curie, 4 Place Jussieuen_US
dc.description.abstractMany new high performance instruments designed for atmospheric measurements and operating on various platforms (balloon, aircraft, satellite) rely heavily on high resolution spectroscopic data relevant to molecular species present in the earth atmosphere. In several cases the quality of the available laboratory data is the limiting factor for taking full advantage of the capabilities of existing or future instruments. However large efforts are devoted in several laboratories to fill the gap. Examples will be presented of this permanent interaction between the remote sensing measurements needs and high resolution infrared studies. Recent balloon and space experiments taking advantage of new spectroscopic line parameters will be described.en_US
dc.format.extent66090 bytes
dc.format.mimetypeimage/jpeg
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titleSOUNDING THE EARTH ATMOSPHERE USING HIGH RESOLUTION INFRARED SPECTROSCOPYen_US
dc.typearticleen_US


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