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dc.contributor.authorBhatt, Megha Upendra
dc.date.accessioned2012-10-08T10:36:41Z
dc.date.available2012-10-08T10:36:41Z
dc.date.issued2012
dc.identifier.urihttp://hdl.handle.net/11858/00-1735-0000-0007-426F-E
dc.description.abstractThe work presented in this thesis is focused on mineralogical studies of the Moon aiming to create maps of iron abundances. We used the data from visible to near-infrared (VISNIR) spectrometers on-board Chandrayaan-1 spacecraft, with our major concentration on the Spectrometer InfraRed-2 (SIR-2) data. The SIR-2 on-ground and in-flight calibrations are discussed. The location of the SIR-2 tracks on the imaging spectrometers, Moon Mineralogy Mapper (M3), and Hyper-Spectral Imager (HySI) is determined by comparing the radiance profiles of the three instruments measured at the same Coordinated Universal Time (UTC) and the same photometric conditions...
dc.format.extent141 S.
dc.language.isoeng
dc.publisherTechn. Univ. Zugl.: Clausthal
dc.subject.ddc549
dc.subject.ddc523.3
dc.subject.ddc550
dc.subject.gokTGG 310
dc.subject.gokTGG 486
dc.subject.swdMond
dc.titleMineralogical analysis and iron abundance estimation of the Moon using the SIR-2, HySI and M3 spectrometers on-board the munar orbiter chandrayaan-1
dc.typemonograph
dc.subject.gokverbalMondbeobachtung, Exploration {Astronomie}
dc.subject.gokverbalZusammensetzung des Mondes {Astronomie}
dc.identifier.doi10.23689/fidgeo-1772
dc.identifier.ppn726156000
dc.type.versionsubmittedVersion
dc.subject.freeEisenmineralien
dc.subject.freeInfrarotspektroskopie
dc.relation.collectionAstronomie, Astrophysik, Weltraumforschung
dc.relation.collectionAstronomie, Astrophysik, Weltraumforschung
dc.description.typethesis


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