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Near and mid-infrared remote sensing of solid planetary surfaces

Arnold, G. (1994) Near and mid-infrared remote sensing of solid planetary surfaces. In: Proceedings of the SSIR, pp. 79-80. Scandinavian Symposium on Infrared and Raman Spectroscopy, Bergen, Norway, 30th May - 1st June 1994.

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Abstract

Infrared spectroscopy is a powerful tool to investigate the mineralogical composition of airless solar system bodies. The information about the surface composition is given by typical minerals and rocks were investigated as functions of particle size, porosity and photometrical characteristics in the near and mid-infrared, respectively. The capabilities and restrictions of these studies are demonstrated by an evaluation of data taken from the Martian surface with the infrared imaging spectrometer on board the Phobos 2.

Document Type:Conference or Workshop Item (Paper)
Additional Information: LIDO-Berichtsjahr=1994, pages=2,
Title:Near and mid-infrared remote sensing of solid planetary surfaces
Authors:
AuthorsInstitution or Email of Authors
Arnold, G.UNSPECIFIED
Date:1994
Journal or Publication Title:Proceedings of the SSIR
Page Range:pp. 79-80
Status:Published
Keywords:Remote sensing, infrared spectroscopy, surface mineralogy
Event Title:Scandinavian Symposium on Infrared and Raman Spectroscopy, Bergen, Norway, 30th May - 1st June 1994
HGF - Research field:UNSPECIFIED
HGF - Program:other
HGF - Program Themes:other
DLR - Research area:UNSPECIFIED
DLR - Program:no assignment
DLR - Research theme (Project):UNSPECIFIED
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Institut für Planetenerkundung
Deposited By: elib DLR-Beauftragter
Deposited On:02 Apr 2006
Last Modified:27 Apr 2009 09:46

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