The lunar photoelectron sheath: A change in trapping efficiency during a solar storm

Author:

Farrell W. M.12,Poppe A. R.32,Zimmerman M. I.142,Halekas J. S.32,Delory G. T.32,Killen R. M.12

Affiliation:

1. NASA Goddard Space Flight Center; Greenbelt Maryland USA

2. NASA Lunar Science Institute, NASA Ames Research Center; Moffett Field California USA

3. Space Sciences Laboratory; The University of California, Berkeley; Berkeley California USA

4. Oak Ridge Associated Universities; Oak Ridge Tennessee USA

Publisher

American Geophysical Union (AGU)

Subject

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

Reference21 articles.

1. The ARTEMIS mission;Angelopoulos;Space Sci. Rev.,2011

2. The coherent Cerenkov radiated power from a group of field-aligned test particles in a magnetoplasma;Farrell;Planet. Space Sci.,1990

3. Coherent Cerenkov emission from the Spacelab-2 electron beam;Farrell;J. Geophys. Res.,1989

4. Solar-Storm/Lunar Atmosphere Model (SSLAM): An overview of the effort and description of the driving storm environment;Farrell;J. Geophys. Res.,2012

5. Photoemission from the lunar surface fines and the lunar photoelectron sheath, Proceedings of the Third Lunar Science Conference, Supplement 3;Feuerbacher;Geochim. Cosmochim. Acta,1972

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