On the Importance of Hiss Waves and Plasma Density for Sculpting the 3D (L-shell, energy, pitch angle) Structure of the Radiation Belts during Quiet Times
Jean-Francois Ripoll1, David Malaspina2, Vivien Loridan1, Michael Denton3, Gregory Cunningham4, Geoffrey D Reeves4, Ondrej Santolik5, Drew L. Turner6, Dr. Xiangning Chu7, J. F. Fennell8, Alexander Drozdov9, Juan Sebastian Cervantes Villa10, Yuri Shprits9, Scott Thaller11, George B Hospodarsky12, William S Kurth13, Craig Kletzing14, John R Wygant15, Michael G Henderson4 and Aleksandr Y Ukhorskiy16, (1)CEA Commissariat à l'Energie Atomique DAM, Arpajon Cedex, France, (2)University of Colorado, Astrophysical and Planetary Sciences Department, Boulder, United States, (3)New Mexico Consortium, Space Science, Los Alamos, NM, United States, (4)Los Alamos National Laboratory, Los Alamos, NM, United States, (5)Institute of Atmospheric Physics, Czech Academy of Sciences, Prague, Czech Republic, (6)The Aerospace Corporation, Los Angeles, CA, United States, (7)University of California Los Angeles, Department of Atmospheric and Oceanic Sciences, Los Angeles, United States, (8)The Aerospace Corporation, Space Sciences Department, EI Segundo, CA, United States, (9)University of California Los Angeles, Los Angeles, United States, (10)Deutsches GeoForschungsZentrum GFZ, 2.8 Magnetospheric Physics, Potsdam, Germany, (11)University of Colorado Boulder, Boulder, United States, (12)University of Iowa, Physics and Astronomy, Iowa City, IA, United States, (13)University of Iowa, Iowa City, IA, United States, (14)University of Iowa, Physics and Astronomy, Iowa City, United States, (15)University of Minnesota, School of Physics and Astronomy, Minneapolis, United States, (16)JHU/APL, Laurel, United States
