Far‐Ultraviolet Photometric Characteristics of JSC‐1A and LMS‐1 Lunar Regolith Simulants: Comparative Investigations With Apollo 10084-Reference-Cited by-同舟云学术

Far‐Ultraviolet Photometric Characteristics of JSC‐1A and LMS‐1 Lunar Regolith Simulants: Comparative Investigations With Apollo 10084

Published:2022-11 Issue:11 Volume:127 Page:
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:JGR Planets

Author:

Gimar C. J.¹²^ORCID,Raut U.¹²³^ORCID,Poston M. J.²³^ORCID,Stevanovic A.⁴^ORCID,Protopapa S.²⁵^ORCID,Greathouse T. K.³^ORCID,Retherford K. D.¹²³^ORCID,Friday J. M.²³,Grimes J. T.²³

Affiliation:

1. Department of Physics and Astronomy University of Texas at San Antonio San Antonio TX USA

2. Center for Laboratory Astrophysics and Space Science Experiments (CLASSE) Space Science and Engineering Division Southwest Research Institute San Antonio TX USA

3. Space Science and Engineering Division Southwest Research Institute San Antonio TX USA

4. Kleberg Advanced Microscopy Center University of Texas at San Antonio San Antonio TX USA

5. Department of Space Studies Southwest Research Institute Boulder CO USA

Funder

National Aeronautics and Space Administration

Southwest Research Institute

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2022JE007508

Reference50 articles.

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5. Britt D. T. &Cannon K. M.(2020).High fidelity lunar highlands and mare regolith simulants: Enabling Tools for lunar surface Exploration and ISRU development presented at the lunar surface Science Workshop held 28‐29 May 2020 (Virtual). LPI Contribution No. 2241 id.5138. Retrieved fromhttps://ui.adsabs.harvard.edu/abs/2020LPICo2241.5138B