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Remote Sounding of the Stratosphere by the Occultation Method: The ORA Experiment

dc.contributor.authorFussen, D.
dc.contributor.authorVanhellemont, F.
dc.contributor.authorBingen, C.
dc.date2003
dc.date.accessioned2018-09-03T11:45:54Z
dc.date.available2018-09-03T11:45:54Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/7050
dc.descriptionThe occultation technique is based on recording of the sun light above the horizon. Its benefit resides in the derivation of an absolute quantity (the slant path optical thickness) through the measurement of a relative signal. The ORA experiment is presented together with the inversion method used to retrieve the atmospheric components.
dc.languageeng
dc.titleRemote Sounding of the Stratosphere by the Occultation Method: The ORA Experiment
dc.typeBook chapter
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.subject.freeOptical Thickness
dc.subject.freeMerit Function
dc.subject.freeTangent Point
dc.subject.freeAerosol
dc.subject.freeOptical Thickness
dc.subject.freeInternational Satellite Cloud Climatology Project
dc.source.titleExploring the Atmosphere by Remote Sensing Techniques
dc.source.page242-262
Orfeo.peerreviewedYes
dc.identifier.doi10.1007/3-540-36536-2_9
dc.source.editorGuzzi, R.


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