Show simple item record

dc.contributor.authorTrompet, L.
dc.contributor.authorMahieux, A.
dc.contributor.authorRistic, B.
dc.contributor.authorRobert, S.
dc.contributor.authorWilquet, V.
dc.contributor.authorThomas, I.R.
dc.contributor.authorVandaele, A.C.
dc.contributor.authorBertaux, J.-L.
dc.contributor.editor
dc.date2016
dc.date.accessioned2016-11-28T11:50:51Z
dc.date.available2016-11-28T11:50:51Z
dc.identifier.isbn978-1-4020-5090-9
dc.identifier.urihttps://orfeo.kbr.be/handle/internal/4557
dc.descriptionThe Solar Occultation in the InfraRed (SOIR) instrument onboard the ESA Venus Express spacecraft, an infrared spectrometer sensitive from 2.2 to 4.3 μm, probed the atmosphere of Venus from June 2006 until December 2014. During this time, it performed more than 750 solar occultations of the Venus mesosphere and lower thermosphere. A new procedure has been developed for the estimation of the transmittance in order to decrease the number of rejected spectra, to check that the treated spectra are well calibrated, and to improve the quality of the calibrated spectra by reducing the noise and accurately normalizing it to the solar spectrum.
dc.languageeng
dc.titleImproved algorithm for the transmittance estimation of spectra obtained with SOIR/Venus Express
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleApplied Optics
dc.source.volume55
dc.source.issue32
dc.source.page9275-9281
Orfeo.peerreviewedYes
dc.identifier.doi10.1364/AO.55.009275


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record