| Paper Number | Title, Author and Affiliation |
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| P-1-1 | MHD Simulation of the Effects of the IMF and Dipole Tilton the Dayside Magnetic Reconnection |
| K. S. Park and T. Ogino | |
| Solar-Terrestrial Environment Laboratory, Nagoya University,Honohara 3-13, Toyokawa, Aichi 442-8507, Japan | |
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| P-1-2 | Mechanism of magnetic hole formation in the magnetosheath |
| K. Tsubouchi, and H. Matsumoto | |
| Research Institute for Sustainable Humanosphere, Kyoto University | |
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| P-1-3 | Structure dimensionality determination using multi-point magnetic field measurements |
| Q. Q. Shi1, C. Shen1, Z.Y. Pu2, M.W. Dunlop3, Z. X. Liu1, A. Balogh3 | |
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1Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, China. 2Institute of Space Physics and Applied Technology, Peking University, Beijing, China. 3Imperial College, London, UK. | |
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| P-1-4 |
Electrostatic solitary waves in the foreshock region of the bow shock: GEOTAIL observations |
| K. Shin1, H. Kojima1, H. Matsumoto1, T. Mukai2 | |
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1Research Institute for Sustainable Humanosphere, Kyoto University, Gokasho, Uji, Kyoto 611-0011, Japan 2Institute of Space and Astronautical Science,3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan | |
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| P-1-5 | INFLUENCE OF ELECTRON NONGYROTROPY ON WAVE INSTABILITIES IN THE EARTH'S BOW SHOCK |
| F. J. R. Simões Júnior1, M. A. E. de Moraes2, and M. V. Alves1 | |
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1Lab. Associado de Plasma, INPE, P.O. BOX 515, 12227-010, S. J. dos Campos, SP, Brazil 2Taubaté University, Taubaté, SP, Brazil | |
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| P-1-6 | Non-thermal Electrons at the Bow Shock: Geotail Observation |
| M. Oka1, T. Terasawa1, Y. Kasaba2, H. Kojima3, M. Fujimoto4, H. Matsumoto3, Y. Saito2 and T. Mukai2 | |
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1The University of Tokyo 2Institute of Space and Astronautical Science, JAXA 3RISH, The University of Kyoto 4Tokyo Institute of Technology | |
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| P-1-7 | Injection Process at quasi-perpendicular shocks: 2D Hybrid Simulation |
| Tooru Sugiyama1, and Masaki Fujimoto2 | |
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1Earth Simulator Center, JAMSTEC 2Tokyo Institute of Technology | |
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| P-1-8 | Adiabaticity breakdown for electrons crossing the stationary/nonstationary front of a collisionless perpendicular shock in supercritical regime |
| P. Savoini and B. Lembege | |
| CETP-UVSQ- IPSL-CNRS, 10-12 avenue de l'Europe, 78140 Velizy, FRANCE | |
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| P-1-9 | Particle simulations of the outer radiation belt during magnetic storm |
| M. S. Nakamura | |
| National Institute of Information and Communications Technology, Koganei,Tokyo, Japan | |
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| P-1-10 |
Simulation study on resonant scattering of relativistic electrons by narrow band whistler mode waves |
| Yuto Katoh and Yoshiharu Omura | |
| Research Institute for Sustainable Humanosphere, Kyoto University, Gokasho, Kyoto, 611-0011 Japan | |
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| P-1-11 | Modeling of two-component thin current sheets inthe Earth's magnetotail: the role of electrostatic effects |
| Victor Popov1, Lev Zelenyi 2, Helmi Malova3,D. Delcourt4, and Surja Sharma5 | |
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1Faculty of Physics, Moscow State University, Moscow, Russia 2Space Research Institute (IKI RAS), Moscow, Russia 3Nuclear Physics Institute of Moscow State University, Moscow, Russia 4CETP-CNRS, Saint-Maur des Fausses, France 5Maryland University, USA | |
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| P-1-12 | Interplanetary magnetic field influence on the jovian magnetosphere |
| E. Belenkaya | |
| Skobeltsyn Institute of Nuclear Physics, Department ofRadiations and Applied Mathematics, Moscow State University, Moscow 119992 Russia | |
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| P-1-13 | An MHD Simulation of Interaction Between the Solar Wind and Jovian Magnetosphere |
| Keiichiro Fukazawa1, Tatsuki Ogino1, and Raymond J. Walker2 | |
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1Solar-Terrestrial Environment Laboratory, Nagoya University, Japan 2Institute of Geophysics and Planetary Physics, University of California, Los Angeles, USA | |
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| P-1-14 | Hybrid Simulations of Ion Cyclotron Waves at Io |
| M.M. Cowee1, N. Omidi2, C.T. Russell1, R.J. Strangeway1 | |
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1Institute of Geophysics and Planetary Physics, University of California, Los Angeles, USA 2SciberNet Inc., Solana Beach, California, USA | |
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| P-1-15 | MHD Simulation of the Saturnian Magnetosphere |
| Shunichi Ogi, Keiichirou Fukazawa and Tatsuki Ogino | |
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Department of Electrical Engineering and Computer Science, Nagoya UniversityAFuro-cho, Chikusa-ku, Nagoya 464-8603, Japan Solar-Terrestrial Environment Laboratory, NagoyaUniversity, 3-13 Honohara, Toyokawa, Aichi 442-8507, Japan | |
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| P-1-16 | 3-D MHD Studies of the night side structure of Mars |
| Y. Kubota1, K. Maezawa1 and H. Jin2 | |
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1Institute of Space and Astronautical Science, Kanagawa, Japan 2National Institute of Information and Communications Technology, Koganei-shi, Tokyo, Japan | |
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| P-1-17 | Global 3d hybrid simulation study of the Martian plasma boundaries |
| A. Boesswetter1, T. Bagdonat1, U. Motschmann1, and K. Sauer2 | |
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1Institute for Theoretical Physics, Technical University of Braunschweig, Germany 2Max-Planck Institute for Solar System Research, Katlenburg-Lindau, Germany | |
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| P-1-18 | Initial Results from an MHD Simulation of Ganymede's Magnetosphere |
| Xianzhe Jia1, Raymond J. Walker1, Margaret G. Kivelson1 and Jon A. Linker2 | |
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1Institute of Geophysics and Planetary Physics and Department of Earth and Space Sciences, University of California, Los Angeles 2Science Applications International Corporation, San Diego. | |
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| P-1-19 | Excitation and trapping of electrostatic waves by ion and electron phase holes |
| Yuan kai, Deng X. H., Zhou meng, Pan ye, and Tang rongxin | |
| Institute of Electronics and Information, Wuhan University, P. R. China | |
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| P-1-20 | Numerical Study of instability in Harris and non-Harris current Sheets |
| Pan ye, Deng X. H., Zhou meng, Yuan kai and Tang rongxin | |
| Institute of Electronics and Information, Wuhan University, P. R. China | |
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| P-1-21 | Study of collisionless reconnection and the role of waves by Cluster, Double Star and Geotail observations and Computer simulations |
| X. H. Deng1, Matsumoto H.2, Kojima H.2, Baumjohann, W.3, Pickett J. S.4, Fazakerley, A. N.5, Andre M.6, Nakamura, R.3, Vaivads, A.6, Gurnett D. A.4, Liu Z. X.7, Coates, A. J.5 | |
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1Institute of Electronics and Information, Wuhan University, P. R. China 2Research Institute for Sustainable Humanosphere, Kyoto University, Japan 3Space Research Institute, Austrian Academy of Sciences, Graz, Austria 4Department of Physics and Astronomy, The University of Iowa, USA 5Mullard Space Science Laboratory, University College London, United Kingdom 6Swedish Institute of Space Physics, Box 537, Uppsala, SE 751 21 Sweden 7CSSAR, CAS, China, Beijing, 100080 China | |
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| P-1-22 | Kinetic simulation study of collisionless magnetic reconnection |
| Zhou meng, Deng X. H., Pan ye, Yuan kai and Tang rongxin | |
| Institute of Electronics and Information, Wuhan University, P. R. China | |
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| P-1-23 | Simulation on solar Type III radio bursts from magnetic reconnection region |
| T. KITAMOTO, J.I. SAKAI, and S.SAITO | |
| Laboratory for Plasma Astrophysics Faculty of Engineering, Toyama University, 3190, Gofuku, Toyama, 930-8555, Japan | |
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| P-1-24 | Magnetic Reconnection at Near-Tail Flank and the Effect on Plasma Convection and Tail Topology |
| J. L. Guo1,2, and Z.X. Liu2 | |
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1Modern Education Technology Center, Peking University, Beijing 100871, China 2Center of Space Science and Application Research, Chinese Academy of Sciences, Beijing, 100080, China | |
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| P-1-25 |
Three Dimensional Flow Structure associated with Spontaneous Fast Magnetic Reconnection Evolution |
| K. Kondoh, M. Ugai, and T. Shimizu | |
| Department of Computer Science, Ehime University, Matsuyama, Ehime, Japan | |
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| P-1-26 | Large-scale three-dimensional plasmoid dynamics associated with the spontaneous fast reconnection model |
| L.Zheng, K.Kondoh, and M.Ugai | |
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Department of Computer Science, Ehime University,Bunkyo-cho 3, Matsuyama, Japan | |
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| P-1-27 | Three-Dimensional Dynamics of Spontaneous Fast Reconnection Evolution |
| M.Shiraishi, K.Kondoh, and M.Ugai | |
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Department of Computer Science, Ehime University, Bunkyo-cho 3, Matsuyama, Ehime, 7908577, Japan | |
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| P-1-28 |
Internal Shocks in the Magnetic Reconnection Jet: 2D MHD Simulations of a Bursty Time-Dependent Reconnection |
| S. Tanuma | |
| Kwasan Observatory, Kyoto University, Yamashina, Kyoto, Japan | |
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| P-1-29 | Roles of Initial Current Carriers in Three-dimensional Magnetic Reconnection |
| X. G. Zhang1,2, Z. W. Ma2, Z. Y. Pu1, Q. Q. Shi3 | |
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1Institute of Space Physics and Applied Technology, Peking University, Beijing, China 2Institute of Plasma Physics, Chinese Academy of Sciences, Hefei, China 3Center of Space Science & Applied Research, Chinese Academy of Sciences, Beijing, China | |
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| P-1-30 | Real-time modeling of the ionosphere using GEDAS/KRM for space weather |
| A. Ieda and Y. Kamide | |
| Solar-Terrestrial Environment Laboratory, Nagoya University, Toyokawa, Aichi, Japan | |
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| P-1-31 | GRID-FDA: A new breed of DDA? |
| James Mc Donald1, Aaron Golden1, and S. Gerard Jennings2 | |
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1Computational Astrophysics Laboratory, National University of Ireland, Galway, Galway, Ireland 2Atmospheric Research Group, National University of Ireland, Galway, Galway, Ireland | |
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| P-1-32 | Development of electromagnetic particle code with adaptive mesh refinement technique: Application to the plasma sheet evolution |
| K. Fujimoto and S. Machida | |
| Department of Geophysics, Graduate School of Science, Kyoto University, Kyoto, Japan | |
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| P-1-33 | Elliptic formulation of discrete Vlasov-Darwin model with the implicit finite-difference representation of particle dynamics |
| L.V. Borodachev | |
| Russia, Moscow State University, Faculty of Physics. | |
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| P-1-34 | CISM-DX: A Tool for Visualizing Space Physics Models and Data |
| Michael Wiltberger1, Robert Wegiel2, Michael Gehmeyr2 | |
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1High Altitude Observatory, National Center For Atmospheric Research, Boulder, CO, USA. 2Laboratory for Atmospheric and Space Physics, University of Colorado,Boulder, CO, USA. | |
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| P-1-35 | Space Plasma Simulations using CIP-MOCCT Method |
| R. TanDokoro, N. Shirataka, K.E.T. Nakamura and M. Fujimoto | |
| Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo, 152-8551 Japan | |
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| P-1-36 | Charge conservation methods for computing current densities in electromagnetic particle-in-cell simulations |
| Takayuki Umeda1, Yoshiharu Omura2, and Hiroshi Matsumoto2 | |
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1Institute of Geophysical and Planetary Physics, University of California, Los Angels, California 90095-1567, USA 2Research Institute for Sustainable Humanosphere, Kyoto University, Uji, Kyoto 611-0011, Japan | |
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| P-1-37 | Coupling Solar Terrestrial Models using Overture and InterComm |
| Charles Goodrich1, John Lyon1,2, and Timothy Guild1 | |
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1Boston University Center for Space Physics, 725 Commonwealth Ave., Boston MA 02215, USA 2Darmouth College, 6127 Wilder Laboratory, Hanover, NH 03755, USA | |
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| P-1-38 | Unstructured Grids and Modelling Alfven Waves in Earth Magnetosphere |
| R. Marchand, J.Y. Lu, K. Kabin R. Rankin, and T. Keeler | |
| Department of Physics, University of Alberta, Edmonton AB, T6G 2J1, Canada |