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Sources and sinks of clay minerals on Mars

Author
MILLIKEN, Ralph E1 ; BISH, David L2
[1] Jet Propulsion Laboratory/California Institute of Technology, Mail Stop 183-301, 4800 Oak Grove Dr., Pasadena, CA 91109, United States
[2] Department of Geological Sciences, Indiana University, 1001 East 10th Street, Bloomington, IN 47405, United States
Conference title
Micro et Nano-Scientiae Mare Magnum
Conference name
International Clay Conference (ICC) (ICC) (14 ; Castellaneta Marina, Taranto 2009-06-14)
Author (monograph)
VALDRE, Giovanni (Editor)1
Association Internationale pour l'Etude des Argiles (AIPEA), Associazione Italiana per lo Studio delle Argille (AISA), International (Organiser of meeting)
[1] Department of Earth and Geo-Environmental Sciences Alma Mater Studiorum, University of Bologna, Italy
Source

Philosophical magazine (2003. Print). 2010, Vol 90, Num 17-18, pp 2293-2308, 16 p ; ref : 38 ref

ISSN
1478-6435
Scientific domain
Crystallography; Condensed state physics
Publisher
Taylor & Francis, Abingdon
Publication country
United Kingdom
Document type
Conference Paper
Language
English
Keyword (fr)
Argile Facteur réflexion Fer Kaolin Minéral Phénomène transport Planète Mars Smectite Spectre IR proche Spectre réflexion Spectre visible 9635
Keyword (en)
Clays Reflectivity Iron Kaolin Minerals Transport processes Mars planet Smectite Near infrared spectrum Reflection spectrum Visible spectra
Keyword (es)
Espectro IR próximo Espectro reflexión
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B90 Other topics on the solar system

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
22922994

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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