dc.contributor.author |
Blaney, D. |
|
dc.contributor.author |
Mouroulis, P. |
|
dc.contributor.author |
Green, R. |
|
dc.contributor.author |
Rodriguez, J. |
|
dc.contributor.author |
Sellar, G. |
|
dc.contributor.author |
Van Gorp, B. |
|
dc.contributor.author |
Wilson, D. |
|
dc.date.accessioned |
2013-10-17T22:22:07Z |
|
dc.date.available |
2013-10-17T22:22:07Z |
|
dc.date.issued |
2011-10-03 |
|
dc.identifier.citation |
European Planetary Science Congress (EPSC) Joint Meeting 2011 La Cité Internationale des Congrès Nantes Métropole, Nantes, France, October 2-7, 2011 |
en_US |
dc.identifier.clearanceno |
11-2581 |
|
dc.identifier.uri |
http://hdl.handle.net/2014/43916 |
|
dc.description.abstract |
In Situ imaging spectroscopy provides a way to address complex questions of geological evolution for both aqueous and igneous processes by mapping mineral composition at the spatial scale of rocks and outcrops. Examination of locations studied by the Mars Exploration Rovers Spirit and Opportunity can provide examples of the potential utility and define the needed measurement requirements. A compact instrument is needed to be able to adequately address these science questions from a rover platform. The Ultra Compact Imaging Spectrometer (UCIS) is an instrument designed to address the science need and implementation constraints. |
en_US |
dc.description.sponsorship |
NASA/JPL |
en_US |
dc.language.iso |
en_US |
en_US |
dc.publisher |
Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011. |
en_US |
dc.subject |
mineralogy sampling |
en_US |
dc.title |
In situ visible to short wavelength imaging spectroscopy with the Ultra Compact Imaging Spectrometer (UCIS): case studies from the Mars Exploration Rovers. |
en_US |
dc.type |
Preprint |
en_US |