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Lunar regolith thermal gradients and emission spectra: Modeling and validation

Abstract:

The retrieval of surface composition from IR measurements of airless bodies requires a model capable of computing the significant thermal gradients present in the top few hundred microns of the regolith. In this study we introduce a model which reproduces most of the features found in controlled experiments made in the simulated lunar environment emission chamber (SLEEC). Although the model presented here is forced by a lower boundary held at a fixed temperature, we conclude that a similar al...

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Publisher copy:
10.1029/2011JE003874

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Role:
Author
Journal:
Journal of Geophysical Research E: Planets
Volume:
116
Issue:
12
Publication date:
2011-01-01
DOI:
ISSN:
0148-0227
Source identifiers:
239785
Language:
English
Pubs id:
pubs:239785
UUID:
uuid:8437c564-6434-495e-ad21-5da519f94efe
Local pid:
pubs:239785
Deposit date:
2013-11-16

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