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Characteristics of infrared data needs for future planetary and cometary observations

dc.contributor.authorMuller, C.
dc.contributor.authorMoreau, D.
dc.contributor.authorRodin, A.V.
dc.date1997
dc.date.accessioned2017-05-22T13:18:39Z
dc.date.available2017-05-22T13:18:39Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/5481
dc.languageeng
dc.titleCharacteristics of infrared data needs for future planetary and cometary observations
dc.typeConference
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleProceedings of SPIE 3090: 12th Symposium and School on High-Resolution Molecular Spectroscopy
dc.source.volume3090
dc.source.page344-348
Orfeo.peerreviewedNo
dc.identifier.doi10.1117/12.267799
dc.identifier.scopus2-s2.0-58649084826
dc.source.editorSinitsa, L.N.
dc.source.editorPonomarev, Y.N.
dc.source.editorPerevalov, V.I.


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