Comparing Magnetic Field Signatures at the Lunar Surface and the Upstream Plasma Environment Using LMS and THEMIS-ARTEMIS
Comparing Magnetic Field Signatures at the Lunar Surface and the Upstream Plasma Environment Using LMS and THEMIS-ARTEMIS
Stephanie K Howard1,2, Jared R Espley3, Robert E Grimm4, Jacob Gruesbeck5, Catherine Johnson6,7, Gregory Delory8, Ian Garrick-Bethell9, Rachel Maxwell2,10, Clive Robert Neal11, Michael E Purucker12, Fiona Simpson13 and David E Stillman14, (1)Howard University, Washington, DC, United States, (2)NASA Goddard Space Flight Center, Greenbelt, United States, (3)Goddard Space Flight Center, Greenbelt, United States, (4)Southwest Research Institute Boulder, Boulder, CO, United States, (5)NASA GSFC, Greenbelt, United States, (6)University of British Columbia, Vancouver, BC, Canada, (7)Planetary Science Institute, Tucson, United States, (8)Heliospace Corp., Berkeley, United States, (9)University of California Santa Cruz, Santa Cruz, United States, (10)University of Maryland Baltimore County, Baltimore, United States, (11)Univ Notre Dame, Notre Dame, United States, (12)NASA Goddard Space Flight Center, Planetary Magnetospheres Laboratory, Greenbelt, MD, United States, (13)Imperial College London, London, United Kingdom, (14)Southwest Research Institute, Boulder, CO, United States