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dc.contributor.authorMahieux, A.
dc.contributor.authorWilquet, V.
dc.contributor.authorDrummond, R.
dc.contributor.authorBelyaev, D.
dc.contributor.authorFederova, A.
dc.contributor.authorVandaele, A.C.
dc.date2009
dc.date.accessioned2016-04-05T13:47:15Z
dc.date.available2016-04-05T13:47:15Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3307
dc.descriptionThe current study describes the determination of the transfer function of an Acousto Optical Tunable Filter from the in-flight solar observations of the SOIR instrument on board Venus Express. An approach is proposed in order to reconstruct the transfer function profile from the analysis of various solar lines. Moreover this technique allows the determination of the evolution of the transfer function as a function of the AOTF radio frequency. © 2009 Optical Society of America.
dc.languageeng
dc.titleA new method for determining the transfer function of an Acousto optical tunable filter
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeFunctions
dc.subject.freeOptical filters
dc.subject.freeProbability density function
dc.subject.freeAcousto-optical tunable filters
dc.subject.freeAnalysis of various
dc.subject.freeRadio frequencies
dc.subject.freeSolar lines
dc.subject.freeSolar observations
dc.subject.freeVenus express
dc.subject.freeTransfer functions
dc.source.titleOptics Express
dc.source.volume17
dc.source.issue3
dc.source.page2005-2014
Orfeo.peerreviewedYes
dc.identifier.doi10.1364/OE.17.002005
dc.identifier.scopus2-s2.0-59749093453


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