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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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|
|Journal or Publication Title:||Proceedings of the SSIR|
|Page Range:||pp. 79-80|
|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|
|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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