ISSS-7 Proceedings

---

Paper Number	Title, Author and Affiliation
P-2-1	Efficient Parallelization of MHD Code and Visualization by VRML
	T. Ogino, K. Fukazawa, H. Sawada, S. Ogi, and M. Nakao
	Solar-Terrestrial Environment Laboratory, Nagoya University,3-13 Honohara, Toyokawa, Aichi 442-8507, Japan
P-2-2	Visualizing earth magnetic flow
	DongSheng Cai, XiaoYang Yan, Wei Li
	Graduate School of System and Information Engineering university of Tsukuba
P-2-3	A Three-Dimensional Visualization System for Real-Time Earth's Magnetosphere Simulator
	Mitsue Den1, Tomoya Ogawa1, Takuhito Kuwabara1, Takashi Tanaka2,3, Igor Goncharenko4, Hiroyoshi Amo5, Yutaka Kanou4, and S. Nallani-Parayil4
	1National Institute of Information and Communications Technology, 4-2-1 Nukuikita, Koganei, Tokyo, 181-8795, JAPAN 2Department of Physics, Kyushu University, 6-10-1, Hakozaki, Higashi-ku, Fukuoka, 812-8581, Japan 3CREST, Japan Science and Technology Agency 43D Incorporated, 1-1 Sakae, Kanagawa-ku, Yokohama, Kanagawa, 221-0052, JAPAN 5NEC Corporation, 2-7-17 Shiba, Minato-ku, Tokyo, 105-0014, JAPAN
P-2-4	Building a 3D Hall MHD model using the Overture framework
	Timothy Guild1, Charles Goodrich1, Viacheslav Merkin1, and John Lyon$^1,^2$
	1Boston University Center for Space Physics, 725 Commonwealth Ave., Boston MA 02215, USA 2Darmouth College, 6127 Wilder Laboratory, Hanover, NH 03755, USA
P-2-5	Grid Computing of Skeleton PIC code on SuperSINET
	Weifeng Tao, Dongsheng Cai
	Graduate School of System and InformationEngineering, University of Tsukuba
P-2-6	Numerical schemes for one-dimensional electrostatic Vlasov code: Comparison between conservative and non-conservative schemes
	Takayuki Umeda1, David Schriver1, and Maha Ashour-Abdalla1,2
	1Institute of Geophysical and Planetary Physics, University of California, Los Angels, California 90095-1567, USA 2Department of Physics and Astronomy, University of California, Los Angels, California 90095-1567, USA
P-2-7	Development of a Parallel Fully Relativistic 3-Dimensional Particle-in-Cell Model of Electron Cyclotron Maser Emission from Brown Dwarfs
	Gregg Hallinan and Aaron Golden
	Computational Astrophysics Laboratory, National University of Ireland Galway, Galway, Ireland
P-2-8	Multi-dimensional Quasineutral Particle/Fluid Simulation Approach for Whistlers
	Martin Lampe1, Glenn Joyce2, Wallace M. Manheimer3, Anatoly Streltsov3, and Gurudas Ganguli1
	1Plasma Physics Division, Naval Research Laboratory, Washington, DC 20375-5346, USA 2George Mason University, Fairfax, VA 22030, USA 3Icarus Research, Inc., Bethesda, MD, USA
P-2-9	Parallel Computation of Particle Codes on Symmetric Multi-Processing Computers
	H. Usui, Y. Omura, Y. Katoh, M. Aoki, Y. Tanimura, and K. Tomita
	Research Institute for Sustainable Humanosphere, Kyoto University, Gokasho, Kyoto, 611-0011 Japan
P-2-10	Validity of the fluid description for ballooning instability onset in the near-Earth collisionless high-β plasma
	Akira Miura
	Deparment of Earth and Planetary Science, University of Tokyo, Tokyo, Japan
P-2-11	The nonlinear particle dynamics in double-humped thin current sheets
	Denis Ovodkov1,Victor Popov2, D. Delcourt3, Helmi Malova4
	1,2Faculty of Physics, Moscow State University, Moscow, Russia 3CETP-CNRS, Saint-Maur des Fausses, France 4Nuclear Physics Institute of Moscow State University, Moscow, Russia
P-2-12	Numerical study of the density ratio effect on the nonlinear beam-plasma interaction
	Tongnyeol Rhee1, Chang-Mo Ryu1, and Peter H. Yoon2
	1Department of Physics, Pohang University of Science and Technology, Pohang, Korea 2Insitute for Physical Science and Technology, University of Maryland, College park, Maryland 20742
P-2-13	Electrostatic waves excited by electron beam in non-thermal plasma
	Quanming Lu and Shui Wang
	School of Earth and Space Sciences, University ofScience and Technology of China, Hefei, Anhui 230026, P. R. China
P-2-14	Nonlinear evolution of electron two-stream instability: Two-dimensional particle simulation
	Takayuki Umeda1, Yoshiharu Omura2, Taketoshi Miyake3, and Hiroshi Matsumoto2
	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 3Toyama Prefectural University, Kosugi, Toyama 930-0398, Japan
P-2-15	EFFECTS OF THE ELECTRON NONGYROTROPY TYPE IN THE BEAM-PLASMA INTERACTIONS
	M. A. E. de Moraes1, M. V. Alves2, and F. J. R. Simões Júnior2
	1Taubaté University, Taubaté, SP, Brazil 2Lab. Associado de Plasma, INPE, P.O. BOX 515, 12227-010, S. J. dos Campos, SP, Brazil
P-2-16	Particle acceleration and magnetic field generationassociated with Weibel instability in relativistic shocks
	K.-I. Nishikawa1, P. Hardee2, C. Hededal3,G. Richardson4, R. Preece5, H. Sol6, and G. J. Fishman7
	1National Space Science and Technology Center, Huntsville, AL 35805 USA 2Department of Physics and Astronomy, The University of Alabama, Tuscaloosa, AL 35487 USA 3Niels Bohr Institute, Department of Astrophysics, Juliane Maries Vej30, 2100 K\o benhavn \O, Denmark 4 Department of Mechanical and Aerospace Engineering University of Alabama in Huntsville Huntsville, AL 35899 USA 5 Department of Physics, University of Alabama in Huntsville, Huntsville, AL 35899 and NSSTC, Huntsville, AL 35805 6 LUTH, Observatore de Paris-Meudon, 5 place Jules Jansen 92195 Meudon Cedex, France 7 NASA-Marshall Space Flight Center, NSSTC, Huntsville, AL 35805
P-2-17	Particle simulation of cyclotron interaction of chorus in a nonuniform magnetic field
	Mitsuru Hikishima1, Satoshi Yagitani1, Isamu Nagano1, Yoshiharu Omura, and Hiroshi Matsumoto2
	1Graduate School of Natural Science and Technology, Kanazawa University, 2-40-20 Kodatsuno, Kanazawa 920-8667, Japan 2Research Institute for Sustainable Humanosphere, Kyoto University, Gokanosho, Uji 611-0011, Japan
P-2-18	Finite amplitude Alfvén wave in a relativistic electron-positron plasma
	T. Hada1, S. Matsukiyo1, V. Muñoz1,2, and M. Ikeda1
	1 Department of Earth System Science and Technology, Kyushu University, Fukuoka 816-8580, Japan 2 Departamento de Física, Facultad de Ciencias,Universidad de Chile, Casilla 653, Santiago, Chile
P-2-19	Modified Two-Stream Instability in a High Mach Number Quasi-Perpendicular Shock Front
	S. Matsukiyo1, and M. Scholer2
	1ESST, Kyushu University,Kasuga, Fukuoka, Japan 2Max-Planck-Institut f…‘r extraterrestrische Physik, Garching, Germany
P-2-20	Electromagnetic lower-hybrid drift instabilities in a bifurcated current sheet model
	Chinook Mok1, Chang-mo Ryu1, Peter H. Yoon2
	1Department of Physics, Pohang University ofScience and Technology, Pohang, Korea 2Institute for Physical Science and Technology, University of Maryland, College Park, Maryland 20742, USA
P-2-21	Solar Wind Parameters at 5.2 AU Predicted by a One-dimensional Magnetohydrodynamic Model
	Chihiro Tao1, Ryuho Kataoka2, Hiroshi Fukunishi1, Yukihiro Takahashi1, and Takaaki Yokoyama3
	1Department of Geophysics, Tohoku University, Sendai, Miyagi, Japan 2National Institute of Information and Communications Technology, Koganei, Tokyo, Japan 3Department of Earth and Planetary Science, University of Tokyo, Bunkyo-ku, Tokyo, Japan
P-2-22	Current Work on a Magnetohydrodynamic Code To Model Pulsar Wind Interactions: The Particular Case of CTB80
	G.Clyne, A.Golden, and S.Bourke
	Computational Astrophysics Laboratory, IT Department, National University of Ireland, Galway, Galway, Ireland
P-2-23	Simulation of Collisionless Damping of Shear Alfvén Waves - Applications to Coronal Heating and Solar Wind Acceleration
	J. I. Sakai1, D. Tsiklauri2, W. Yamamura1, M. Hayashi1, S. Saito1, H. Washimi3 and G. Vekstein4
	1Laboratory for Plasma Astrophysics Faculty of Engineering, Toyama University, 3190, Gofuku, Toyama, 930-8555, Japan 2 Space Technology,Solar & Space Phys. University of Salford, Manchester, M5 4WT, UK 3Institute of Geophysics and Planetary Physics, University of California, Riverside, USA 4School of Physics and Astronomy, The University of Manchester, Manchester M60 1QD, UK
P-2-24	The emission of electromagnetic waves during the coalescence of two parallel current loops in solar flares
	Shinji Saito and Jun-ichi Sakai
	Laboratory for Plasma Astrophysics, Faculty of Engineering, Toyama University, 3190, Gofuku, Toyama, Japan 930-8555
P-2-25	Broad Radio Bursts and Fine Structures During the Great Solar Events in Late October 2003
	Shujuan Wang
	National Astronomical Observatories, CAS, Beijing 100012, P. R. China
P-2-26	Simulation on Solar Type II Radio Bursts associated with Coronal Mass Ejections
	T. MORI, J.I. SAKAI, and S.SAITO
	Laboratory for Plasma Astrophysics Faculty of Engineering, Toyama University, 3190, Gofuku, Toyama, 930-8555, Japan
P-2-27	Three-dimensional magnetohydrodynamic simulation of the sun-solar wind system on the dodecahedronal gridpoint model
	Tomomi Suzuki1,3, Takashi Tanaka2,3
	1Graduate School of Sciences, Kyushu University 2Faculty of scienses, Kyushu University 3CREST, Japan Science and Technology agency
P-2-28	Three-dimensional Hydrodynamic Code for Interplanetary Shock Wave
	Tomoya Ogawa1, Mitsue Den1, and Takashi Tanaka2,3
	1Space Simulation Group, National Institute of Information and Communications Technology, 4-2-1 Nukuikita-machi, Koganei, Tokyo 184-8795, Japan 2Department of Earth and Planetary Sciences, Kyushu University, 6-10-1 Hakozaki, Higashi-ku, Fukuoka 812-8581, Japan 3CREST, Japan Science and Technology Agency
P-2-29	A 3D Hall-MHD study of reconnection and filament formation from magnetic flux emergence in the sun: Preliminary results
	Z.G. Zhou1, C.J. Xiao1, Z.W. Ma2, Z.Y. Pu3 and J.X. Wang1
	1National Astronomical Observatories, CAS, China 2Institute of plasma physics, CAS, China 3School of Earth and space Sciences, Peking University, China
P-2-30	Three-Dimensional MHD Simulation of Magnetosphere-Ionosphere Coupling
	Kazuhide Sawada and Tatsuki Ogino
	Department of Electrical Engineering and Computer Science, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8603, Japan Solar-Terrestrial Environment Laboratory, Nagoya University, 3-13 Honohara, Toyokawa, Aichi 442-8507, Japan
P-2-31	An new approach to the process of the magnetosphere--ionosphere coupling in global MHD simulations
	A. Yoshikawa1 and H. Nakata2
	1Department of Earth and Planetary Sciences, Kyushu University, Fukuoka, Japan 2Graduate school of Science and Technology, Chiba University, Chiba, Japan
P-2-32	Role of the Magnetospheric and Ionospheric Currents in Generation of the Equatorial Scintillations During Geomagnetic Storms
	L. Biktash
	IZMIRAN, Troitsk, Moscow Region, Russia
P-2-33	Problems of Dst index Simulation
	L. Biktash (Sizova)
	Institute of Terrestrial Magnetism. Ionosphere and Radio Wave Propagation, Troitsk, Moscow Region, Russia
P-2-34	A Numerical Simulation of a Geomagnetic Sudden Commencement
	S. Fujita1,3 and T. Tanaka2,3
	1Meteorological College, Kashiwa, Chiba Japan 2Department of Geophysics and Planetary Sciences, Kyushu University, Fukuoka Japan 3CREST, Japan Science and Technology Agency
P-2-35	Modeling the Kinetic Transport of Electrons throughout the Earth's Global Magnetosphere
	D. Schriver1, M. Ashour-Abdalla1, L. Zelenyi2, T. Gombosi3, A. Ridley3, D. De Zeeuw3, G. Toth3 and G. Monostori4
	1Institute of Geophysics and Planetary Physics, UCLA, Los Angeles, California, USA 2Space Research Institute, Russian Academy of Science, Moscow 3Space Physics Research Laboratory, University of Michigan 4Eotvos University, Budapest, Hungary
P-2-36	Modeling Solar Wind Particles Transport Into the Plasma Sheet With Test Particle Simulation
	Ding Li, Richard Marchand, Konstantin Kabin and Robert Rankin
	Department of Physics, University of Alberta, Edmonton, Alberta, Canada
P-2-37	Simulation of the entry of solar energetic protons into the magnetosphere
	Hironori Shimazu1 and Takashi Tanaka2
	1Applied Research and Standards Department,National Institute of Information and Communications Technology,Koganei, Tokyo 184-8795, Japan, and CREST, JST. 2Department of Earth and Planetary Sciences, Kyushu University, Hakozaki, Higashi-ku, Fukuoka 812-8581, Japan, and CREST, JST.
P-2-38	Modeling the Inner Magnetosphere with the Coupled Rice Convection Model -- Equilibrium Code
	C. Lemon$^{1*}$, T. W. Hill1, S. Sazykin1, R. W. Spiro1, F. R. Toffoletto1, R. A. Wolf1, J. Birn2 and M. Hesse3
	1Department of Physics and Astronomy, Rice University, Houston, Texas, USA 2Los Alamos National Laboratory, Los Alamos, New Mexico, USA 3NASA Goddard Spaceflight Center, Greenbelt, Maryland, USA $^*$Now at The Aerospace Corporation, Los Angeles, California, USA
P-2-39	Electrostatic Ion Cyclotron and Ion Acoustic waves in Auroral Plasma
	R. V. Reddy1, S. V. Singh1, G. S. Lakhina1,2 and R. Bharuthram3
	1Indian Institute of Geomagnetism, New Panvel, Navi Mumbai - 410218, India 2Research Institute for Sustainable Humanosphere, Kyoto University, Gokasho, Uji, Kyoto 611-0011, Japan 3University of KwaZulu-Natal, Durban 4000, South Africa
P-2-40	Colliding Convection Model of the Theta Aurora
	T. Tanaka1,3 and T. Obara2,3
	1Department of Geophysics and Planetary Sciences, Kyushu University, Fukuoka Japan 2National Institute of Information and Communication Technology, Koganei, Tokyo, Japan 3CREST, Japan Science and Technology Agency

---

| Back to Proceedings Main Page | Top Page |