Lunar surface processes - Report of the 12054 consortiumA variety of lunar surface phenomena were studied using a well-characterized glass-coated ilmenite basalt, 12054, which had a simple surface residence history. Surface processes related to the following effects were studied: microcraters, solar flare and cosmic ray tracks, cosmogenic Al-26, solar wind sputtering, accreta or accretionary material, solar wind implanted noble gases, and loose dust accumulation.
Document ID
19790055227
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Hartung, J. B. (Centre d'Etudes et de Recherches Toulouse, France)
Hauser, E. E. (New York, State University Stony Brook, N.Y., United States)
Horz, F. (Centre d'Etudes et de Recherches Toulouse, France)
Morrison, D. A. (Centre d'Etudes et de Recherches Toulouse, France)
Schonfeld, E. (Centre d'Etudes et de Recherches Toulouse, France)
Zook, H. A. (NASA Johnson Space Center Houston, Tex., United States)
Mandeville, J.-C. (ONERA Centre d'Etudes et de Recherches de Toulouse, Toulouse, France)
Mcdonnell, J. A. M. (Kent, University Canterbury, United Kingdom)
Schaal, R. B. (Lockheed Electronics Co., Inc. Houston, Tex., United States)
Zinner, E. (Washington University St. Louis, Mo., United States)