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High-resolution CASSINI-VIMS mosaics of Titan and the icy Saturnian satellites

Jaumann, R. and Stephan, K. and Brown, R. H. and Buratti, B. J. and Clark, R. N. and McCord, T. B. and Coradini, A. and Capaccioni, F. and Filacchione, G. and Cerroni, P. and Baines, K. H. and Bellucci, G. and Bibring, J.-P. and Combes, M. and Cruikshank, D. P. and Drossart, P. and Formisano, V. and Langevin, Y. and Matson, D. L. and Nelson, R. M. and Nicholson, P. D. and Sicardy, B. and Sotin, C. and Soderbloom, L. A. and Griffith, C. and Matz, K.-D. and Roatsch, Th. and Scholten, F. and Porco, C. C. (2006) High-resolution CASSINI-VIMS mosaics of Titan and the icy Saturnian satellites. Planetary and Space Science, 54, pp. 1146-1155. Elsevier. doi: 10.1016/j.pss.2006.05.034. ISSN 0032-0633.

Full text not available from this repository.

Abstract

The Visual Infrared Mapping Spectrometer (VIMS) onboard the CASSINI spacecraft obtained new spectral data of the icy satellites of Saturn after its arrival at Saturn in June 2004. VIMS operates in a spectral range from 0.35 to 5.2 mm, generating image cubes in which each pixel represents a spectrum consisting of 352 contiguous wavebands. As an imaging spectrometer VIMS combines the characteristics of both a spectrometer and an imaging instrument. This makes it possible to analyze the spectrum of each pixel separately and to map the spectral characteristics spatially, which is important to study the relationships between spectral information and geological and geomorphologic surface features. The spatial analysis of the spectral data requires the determination of the exact geographic position of each pixel on the specific surface and that all 352 spectral elements of each pixel show the same region of the target. We developed a method to reproject each pixel geometrically and to convert the spectral data into map projected image cubes. This method can also be applied to mosaic different VIMS observations. Based on these mosaics, maps of the spectral properties for each Saturnian satellite can be derived and attributed to geographic positions as well as to geological and geomorphologic surface features. These map-projected mosaics are the basis for all further investigations.

Item URL in elib:https://elib.dlr.de/45051/
Document Type:Article
Title:High-resolution CASSINI-VIMS mosaics of Titan and the icy Saturnian satellites
Authors:
AuthorsInstitution or Email of AuthorsAuthor's ORCID iDORCID Put Code
Jaumann, R.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Stephan, K.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Brown, R. H.Department Planetary Science and LPL, University of AZ, Tucson, AZ, USAUNSPECIFIEDUNSPECIFIED
Buratti, B. J.Jet Propulsion Laboratory, Pasadena, CA, USAUNSPECIFIEDUNSPECIFIED
Clark, R. N.USGS, Denver Federal Center, Denver, CO, USAUNSPECIFIEDUNSPECIFIED
McCord, T. B.Planetary Science Institute, Winthrop, WA, USAUNSPECIFIEDUNSPECIFIED
Coradini, A.Istituto Fisica Spazio Interplanetario, CNR, Roma, ItalyUNSPECIFIEDUNSPECIFIED
Capaccioni, F.Instituto di Astrofisica Spaziale, Roma, ItalyUNSPECIFIEDUNSPECIFIED
Filacchione, G.Instituto di Astrofisica Spaziale, Roma, ItalyUNSPECIFIEDUNSPECIFIED
Cerroni, P.Instituto di Astrofisica Spaziale, Roma, ItalyUNSPECIFIEDUNSPECIFIED
Baines, K. H.Jet Propulsion Laboratory, Pasadena, CAUNSPECIFIEDUNSPECIFIED
Bellucci, G.Istituto Fisica Spazio Interplanetario, CNR, Roma, ItalyUNSPECIFIEDUNSPECIFIED
Bibring, J.-P.Universite de Paris Sud-Orsay, Orsay Cedex, FranceUNSPECIFIEDUNSPECIFIED
Combes, M.Observatoire de Paris-Meudon, Meudon Cedex, FranceUNSPECIFIEDUNSPECIFIED
Cruikshank, D. P.NASA Ames Research Center, Astrophysics Branch, Moffett Field, CA, USAUNSPECIFIEDUNSPECIFIED
Drossart, P.Observatoire de Paris-Meudon, Meudon Cedex, FranceObservatoire de Paris-Meudon, Meudon Cedex, FranceUNSPECIFIEDUNSPECIFIED
Formisano, V.Istituto Fisica Spazio Interplanetario, CNR, Roma, ItalyUNSPECIFIEDUNSPECIFIED
Langevin, Y.Universite de Paris Sud-Orsay, Orsay Cedex, FranceUNSPECIFIEDUNSPECIFIED
Matson, D. L.Jet Propulsion Laboratory, Pasadena, CAUNSPECIFIEDUNSPECIFIED
Nelson, R. M.Jet Propulsion Laboratory, Pasadena, CAUNSPECIFIEDUNSPECIFIED
Nicholson, P. D.Cornell University, Ithaca, NY, USAUNSPECIFIEDUNSPECIFIED
Sicardy, B.Observatoire de Paris-Meudon, Meudon Cedex, FranceUNSPECIFIEDUNSPECIFIED
Sotin, C.University of Nantes, Nantes Cedex, FranceUNSPECIFIEDUNSPECIFIED
Soderbloom, L. A.US Geological Survey, Flagstaff, AZ, USAUNSPECIFIEDUNSPECIFIED
Griffith, C.Lunar and Planetary Laboratory and Stewart Observatory, University of Arizona, Tucson, AZ, USAUNSPECIFIEDUNSPECIFIED
Matz, K.-D.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Roatsch, Th.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Scholten, F.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Porco, C. C.Space Science Institute, Boulder, USAUNSPECIFIEDUNSPECIFIED
Date:2006
Journal or Publication Title:Planetary and Space Science
Refereed publication:Yes
Open Access:No
Gold Open Access:No
In SCOPUS:No
In ISI Web of Science:Yes
Volume:54
DOI:10.1016/j.pss.2006.05.034
Page Range:pp. 1146-1155
Publisher:Elsevier
ISSN:0032-0633
Status:Published
Keywords:Cassini, VIMS, Imaging spectroscopy, Saturnian satellites, Map projection, Mosaics
HGF - Research field:Aeronautics, Space and Transport (old)
HGF - Program:Space (old)
HGF - Program Themes:W EW - Erforschung des Weltraums
DLR - Research area:Space
DLR - Program:W EW - Erforschung des Weltraums
DLR - Research theme (Project):W - Vorhaben CASSINI (old)
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Planetary Geology
Deposited By: Pieth, Susanne
Deposited On:20 Oct 2006
Last Modified:27 Apr 2009 13:09

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