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dc.contributor.authorFussen, D.
dc.contributor.authorVanhellemont, F.
dc.contributor.authorBingen, C.
dc.date2002
dc.date.accessioned2017-05-03T12:21:54Z
dc.date.available2017-05-03T12:21:54Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/5207
dc.descriptionWe present a general analysis of the error budget in the spectral inversion of atmospheric radiometric measurements. By focussing on the case of an occultation experiment, we simplify the problem through a reduced number of absorbers in a linearized formalism. However, our analysis is quite general and applies to many other situations. For a spectrometer having an infinite spectral resolution, we discuss the origin of systematic and random errors. In particular, the difficult case of aerosols is investigated and several inversion techniques are compared. We underline the importance of carefully simulating the spectral inversion as a function of the target constituent to be retrieved, and the required accuracy level.
dc.languageeng
dc.titleOptimal spectral inversion of atmospheric radiometric measurements in the near-UV to near-IR range: A case study
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeComputational methods
dc.subject.freeError analysis
dc.subject.freeFunctions
dc.subject.freeInfrared radiation
dc.subject.freeMatrix algebra
dc.subject.freeRadiometry
dc.subject.freeRandom processes
dc.subject.freeSpectrometers
dc.subject.freeSpectrum analysis
dc.subject.freeUltraviolet radiation
dc.subject.freeError budget
dc.subject.freeRadiometric measurements
dc.subject.freeSpectral inversion
dc.subject.freeSpectral resolution
dc.subject.freeIntegrated optics
dc.source.titleOptics Express
dc.source.volume10
dc.source.issue1
dc.source.page70-82
Orfeo.peerreviewedYes
dc.identifier.doi10.1364/OE.10.000070
dc.identifier.scopus2-s2.0-1342283971


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