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:

Authors	Institution or Email of Authors
Arnold, G.

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:

no assignment

HGF - Program Themes:

no assignment

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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