SM31B:
Dawn-Dusk Asymmetries in Solar Wind-Magnetosphere-Ionosphere Systems I Posters
Wednesday, 17 December 2014: 8:00 AM-12:20 PM
Chairs: Colin Forsyth, Mullard Space Science Lab., Dorking, United Kingdom and Matthew G Taylor, ESTEC, Noordwijk, 2201, Netherlands
Primary Conveners: Stein Haaland, Max-Planck Inst/Univ Bergen, Katlenburg-Lindau, Germany
Co-conveners: Colin Forsyth, University College London, London, United Kingdom
OSPA Liaisons: Andrei Runov, UCLA, Los Angeles, CA, United States
Abstracts Submitted to this Session:
The Effect of the Ion Gyro Motion to Nonlinear Processes of the Kelvin-Helmholtz Instability
Satoshi Ueno1, Takayuki Umeda1, Takuma Nakamura2 and Shinobu Machida1, (1)Nagoya University, Nagoya, Japan, (2)Los Alamos National Laboratory, Plasma Theory and App, Los Alamos, NM, United States
Dayside Magnetopause Location During Radial Interplanetary Magnetic Field Periods
Hui Wang1,2, Tao Huang2, Jih-Hong Shue3 and Aaron J Ridley1, (1)Univ Michigan, Ann Arbor, MI, United States, (2)School of Electronic Information, Wuhan University, Dept. of Space Physics, Wuhan, China, (3)NCU National Central University of Taiwan, Jhongli, Taiwan
Global Plasmaspheric Electron Density Simulations of Pre-dawn and Post-dusk Geomagnetic Events Observed by the Van Allen Probes
Sebastian De Pascuale1, Vania Jordanova2, Jerry Goldstein3 and Craig Kletzing1, (1)University of Iowa, Iowa City, IA, United States, (2)Los Alamos National Laboratory, Los Alamos, NM, United States, (3)Southwest Research Institute San Antonio, San Antonio, TX, United States
Using Auroral Asymmetries to Test MHD Models
Patricia H Reiff1, William James Longley1, Nikolai Ostgaard2 and Jone Peter Reistad3, (1)Rice University, Houston, TX, United States, (2)University of Bergen, Birkeland Centre for Space Science, Bergen, Norway, (3)University of Bergen, Bergen, Norway