Session Chairs: | Bertrand Lembège, Gurbax Lakhina, Iku Shinohara |
Poster Session
HP5.1 Origin Of Gyrotropic/Non Gyrotropic Ion Populations In The Earth's Quasi-Perpendicular Ion Foreshock: Full-Particle 2D Simulation Results
P. Savoini1, B. Lembege2
1LPP - Ecole Polytechnique - UPMC, Palaiseau, France
2LATMOS - CNRS - UVSQ, Guyancourt, France
HP5.2 WAVE EMISSIONS FROM THE LOWER-HYBRID TO THE ELECTRON CYCLOTRON FREQUENCY DUE TO REFLECTED IONS WITHIN THE FRONT OF QUASIPERPENDICULAR SUPERCRITICAL SHOCKS
L. Muschietti1,2, B. Lembege2
1SSL, University of California at Berkeley, Berkeley, CA, United States
2LATMOS-IPSL-UVSQ-CNRS, Guyancourt, France
HP5.3 IMPACT OF PICK-UP IONS ON THE NONSTATIONARITY AND THE MICROSTRUCTURES OF A PERPENDICULAR SUPERCRITICAL SHOCK: FULL PIC SIMULATIONS
Z. Yang1, B. Lembege2, Q. Lu3
1National Space Science Center, Chinese Academy of Sciences, Beijing, China
2LATMOS/IPSL/UVSQ/CNRS, Guyancourt, France
3SESS, Univ. Science and Technology of China, Hefei, China
HP5.4 ION DISTRIBUTIONS IN THE EARTH'S FORESHOCK REGION: HYBRID-VLASOV SIMULATIONS AND SPACECRAFT OBSERVATIONS
Y. Kempf1,2, O. Gutynska3, D. Pokhotelov1, L. B. Wilson III3, B. M. Walsh3, S. von Alfthan2, D. G. Sibeck3, M. Palmroth2
1Department of physics, University of Helsinki, Helsinki, Finland
2Earth observation unit, Finnish Meteorological Institute, Helsinki, Finland
3Goddard Space Flight Center, Greenbelt, Maryland, USA
HP5.5 CLUSTER-C1 OBSERVATIONS OF NON-TRAIN MAGNETIC DECREASES IN THE SOLAR WIND AT 1 AU
T. Xiao, A. Tian, Q. Shi
School of Space Science and Physics, Shandong University at Weihai, Weihai, China
HP5.6 INITIAL RESPONSES OF MAGNETOSPHERIC PLASMA FLOWS TO THE DYNAMIC PRESSURE ENHANCEMENTS
X. Shen1, Q. Shi1, A. Tian1, S. Fu2, Q. Zong2, Z. Pu2
1School of Space Science and Physics, Shandong university, Weihai, China
2Institute of Space Physics and Applied Technology, Peking University, Beijing, China
HP5.7 POLAR CAP ARCS CORRELATED WITH SOLAR WIND ENTRY AT THE HIGH LATITUDE MAGNETOSPHERE
B. Mailyan1,2, Q. Q. Shi1, X. Gou1
1School of Space Science and Physics, Shandong university, Weihai, China
2Cosmic Ray Division, Yerevan Physics Institute, Yerevan, Armenia
HP5.8 SOLAR WIND PENETRATION INTO THE HIGH-LATITUDE MAGNETOSPHERE: CLUSTER OBSERVATIONS
X. C. Gou, Q. Q. Shi
Shandong University, Weihai, China
HP5.9 STATISTICAL STUDY AND PARTICLE SIMULATIONS ABOUT THE LOW FREQUENCY COMPORNENT OF BEN OBSERVED BY GEOTAIL SPACECRAFT
T. Miyake1, S. Nagayasu1, H. Nakada1, M. Okada2, H. Usui3, Y. Omura4
1Toyama Prefectural University, Toyama, Japan
2National Institute Polar Research, Tachikawa, Japan
3Kobe University, Kobe, Japan
4RISH, Kyoto University, Uji, Japan
HP5.10 3-D GLOBAL HYBRID SIMULATIONS OF THE MAGNETOSPHERE DYNAMICS
S. Lu1, Y. Lin2, X. Wang2, Q. Lu1, S. Wang1
1Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei, China
2Department of Physics, Auburn University, Auburn, Alabama, USA
HP5.11 CHARACTERISTICS OF DAYSIDE MAGNETOSPHERIC FLOWS DURING SOLAR WIND DYNAMIC PRESSURE PULSE
A. Tian, X. Shen, Q. Shi
Shandong University(weihai), Weihai, China
HP5.12 ESTIMATION OF WAVE FREQUENCY AND AZIMUTHAL WAVENUMBER OF HIGH-M ULF WAVES BY ST-5 SATELLITE OBSERVATIONS AT LOW ALTITUDES
P. J. Chi1, G. Le2
1Department of Earth, Planetary, and Space Sciences, UCLA, Los Angeles, CA, United States
2Space Weather Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD, United States
HP5.13 STATISTICAL STUDY OF LION ROAR EMISSIONS OBSERVED BY THE CLUSTER SPACECRAFT
V. Krupar1, J. Soucek1, O. Santolik1,2
1Institute of Atmospheric Physics ASCR, Prague, Czech Republic
2Charles University, Prague, Czech Republic