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Classification of Mars Analogue Mixtures and End-Member Minerals Using Self-Organizing Maps

Roush, T. L. and Helbert, J. and Hogan, R. C. and Maturilli, A. (2007) Classification of Mars Analogue Mixtures and End-Member Minerals Using Self-Organizing Maps. In: Lunar and Planetary Science XXXVIII, 1338, abstract#1291. Lunar and Planetary Institute. 38th Lunar and Planetary Science Conference, 2007-03-12 - 2007-03-16, Houston, TX, USA. ISSN 1540-7845

Full text not available from this repository.

Abstract

Emissivity spectra of pure materials and their mixtures are statistically clustered using self-organizing maps. The results exhibit distinct segregation of coarse-grain from fine-grain size samples and primary materials from their potential alteration products.

Document Type:Conference or Workshop Item (Poster)
Title:Classification of Mars Analogue Mixtures and End-Member Minerals Using Self-Organizing Maps
Authors:
AuthorsInstitution or Email of Authors
Roush, T. L.NASA Ames Research Center, Moffett Field, California, USA
Helbert, J.UNSPECIFIED
Hogan, R. C.Bay Area Environmental Research Institute
Maturilli, A.UNSPECIFIED
Date:13 March 2007
Journal or Publication Title:Lunar and Planetary Science XXXVIII
Refereed publication:No
In SCOPUS:No
In ISI Web of Science:No
Volume:1338
Page Range:abstract#1291
Publisher:Lunar and Planetary Institute
Series Name:LPI Contribution
ISSN:1540-7845
Status:Published
Keywords:Mars, Emissivity spectra, Self-Organising Maps
Event Title:38th Lunar and Planetary Science Conference
Event Location:Houston, TX, USA
Event Type:international Conference
Event Dates:2007-03-12 - 2007-03-16
Organizer:Lunar and Planetary Institute
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 Vergleichende Planetologie (old)
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Planetary Physics
Deposited By: Stefanie Hempel
Deposited On:15 Jan 2008
Last Modified:27 Apr 2009 14:36

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