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A new experimental setup for making thermal emission measurements in a simulated lunar environment

Abstract:

One of the key problems in determining lunar surface composition for thermal-infrared measurements is the lack of comparable laboratory-measured spectra. As the surface is typically composed of fine-grained particulates, the lunar environment induces a thermal gradient within the near sub-surface, altering the emission spectra: this environment must therefore be simulated in the laboratory, considerably increasing the complexity of the measurement. Previous me...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1063/1.4769084

Authors


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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Oxford college:
St Cross College
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Oxford college:
Exeter College
Role:
Author
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Publisher:
AIP Publishing Publisher's website
Journal:
Review of Scientific Instruments Journal website
Volume:
83
Issue:
12
Pages:
124502
Publication date:
2012-12-26
Acceptance date:
2012-11-12
DOI:
EISSN:
1089-7623
ISSN:
0034-6748
Pmid:
23278007
Source identifiers:
375639
Language:
English
Keywords:
Pubs id:
pubs:375639
UUID:
uuid:99c81d9d-0ad0-4be4-8083-b99553d063c7
Local pid:
pubs:375639
Deposit date:
2018-04-04

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