Computer Simulation of Space Plasmas

T. Sato

ISBN 10: 9401088500 / ISBN 13: 9789401088503

Editore: Springer Netherlands, 2011

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Druck auf Anfrage Neuware - Printed after ordering - Computer simulation is now widely recognized as a powerful tool and useful method at the current stage of research in space plasma physics. The expected role of computer simulation is to bridge the existing gap between theories and experiments/observations and to give a profound physical insight into highly tangled and nonlinearly coupled space plasma phenomena. One of the goals of space plasma physics in 1980's and 1990's is to elucidate the quantitative causal relationships of global and local energy flows in space plasma environment and establish the space plasma physics via cooperative studies among three important elements of observations, theories and computer simulations. Based on such recognition, Dr. M. Ashour-Abdalla (UCLA/USA), Dr. R. Gendrin (CNET/FRANCE) and both of us met together at the 20th General Assembly of URSI at Washington D. C. in 1981 to discuss what we should do and what we could do, reaching a conclusion that it is time to establish an International School of Space Simulations (ISSS). The objectives of the ISSS thus organized are firstly to educate and stimulate graduate students and young sCientists, secondly to exchange information on updated simulation techniques and thirdly to have mutual discussions among observational, theoretical and simulational scientists in the field of space physics. The first ISSS were organized by Prof. P. Coleman, Prof. T. Obayashi, Dr. H. Okuda in addition to the above four members. The first ISSS was held at Kansai Seminar House in Kyoto from Nov. I to Nov. 12, 1982.

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Dati bibliografici

• Titolo: Computer Simulation of Space Plasmas
• Editore: Springer Netherlands
• Data di pubblicazione: 2011
• Lingua: Inglese
• ISBN 10: 9401088500
• ISBN 13: 9789401088503
• Rilegatura: Taschenbuch
• Condizione: Neu
• Dimensioni: 235 L x 155 A x 22 P (millimetri) 235 millimetri di larghezza per 155 millimetri di altezza per 22 millimetri di profondità
• Peso: 598 grammi

Descrizione articolo

Riassunto

Computer simulation is now widely recognized as a powerful tool and useful method at the current stage of research in space plasma physics. The expected role of computer simulation is to bridge the existing gap between theories and experiments/observations and to give a profound physical insight into highly tangled and nonlinearly coupled space plasma phenomena. One of the goals of space plasma physics in 1980's and 1990's is to elucidate the quantitative causal relationships of global and local energy flows in space plasma environment and establish the space plasma physics via cooperative studies among three important elements of observations, theories and computer simulations. Based on such recognition, Dr. M. Ashour-Abdalla (UCLA/USA), Dr. R. Gendrin (CNET/FRANCE) and both of us met together at the 20th General Assembly of URSI at Washington D. C. in 1981 to discuss what we should do and what we could do, reaching a conclusion that it is time to establish an International School of Space Simulations (ISSS). The objectives of the ISSS thus organized are firstly to educate and stimulate graduate students and young sCientists, secondly to exchange information on updated simulation techniques and thirdly to have mutual discussions among observational, theoretical and simulational scientists in the field of space physics. The first ISSS were organized by Prof. P. Coleman, Prof. T. Obayashi, Dr. H. Okuda in addition to the above four members. The first ISSS was held at Kansai Seminar House in Kyoto from Nov. I to Nov. 12, 1982.

Contenuti

I Particle Simulations.- to Particle Simulation Models and Other Application to Electrostatic Plasma Waves.- I: Introduction to Particle Simulation Models in Plasma Physics.- 1. Introduction.- 2. Electrostatic Particle Simulation Models.- 3 Numarical Methods Using Finite-Size Particles.- II: Appplication of Particle Simulation to Electrostatic Ion Cyclotron Waves on Auroral Field Lines.- 1. Introduction.- 2. Results of Simulation Without a Source.- 3. Results of Simulation With a Source.- 4. Formation of Auroral Arc Elements.- 5. Discussions.- References.- Particle Simulation of Electromagnetic Waves and Its Application to Space Plasmas.- 1. Introduction.- 2. Elementary Concepts and Models in Particle Simulations.- 3. Particle Code valid for both Electromagnetic and Electrostatic Wave Models.- 4. Long-Time-Scale Code for Monochromatic Whistler Interaction.- 5. Diagnostic Tools.- 6. Application to Space Plasma Wave Phenomena.- 7. Concluding Remarks.- References.- Relativistic Code Applied to Radiation Generation.- 1. Introduction.- 2. Boundary Conditions for Outgoing Electromagnetic Waves.- 3. Electron Cyclotron Maser Instabilities.- References.- Modern Development in Particle Simulation.- 1. Introduction.- 2. Implicit Time Integration.- 3. Moment Method.- 4. Direct Method.- 5. Conclusions.- Refereces.- II MHD Simulations.- Principles of Magnetohydrodynamic Simulation in Space Plasmas.- 1. Introduction.- 2. MHD Equations.- 3. Guiding Principles of MHD Simulation.- 4. Local MHD Model.- 5. Global MHD Model.- 6. Boundary Conditions.- 7. Simulation Code and Diagnostics.- 8. Closing Remarks.- References.- MHD Modelling of the Earth’s Magnetosphere.- 1. Introduction.- 2. Global MHD Model.- 3. Numarical Methods.- 4. Results.- 5. Conclusion.- References.- Numerically-Simulated Formation and Propagation of Interplanetary Shocks.- 1. Introduction.- 2. Numerical Methods and Mathematical Models.- 3. Computation Procedures and Physical Results.- 4. Concluding Remarks.- References.- Anomalous Transport by Kelvin-Helmholtz Instabilities.- 1. Introduction.- 2. Basic Equations and Models.- 3. Numerics.- 4. Numerical Results.- 5. Summary and Discussion.- References.- III Other-Method Simulations.- Particle Behavior in the Magnetosphere.- 1. Introduction.- 2. Basic Equations and Physical Assumptions.- 3. Model Inputs.- 4. Program Logic and Numerical Methods.- 5. Review of Results.- 6. Concluding Comments.- References.- Hybrid Simulation Techniques Applied to the Earth’s Bow Shock.- 1. Introduction.- 2. Numerical Methods.- 3. Applications.- 4. Summary.- References.- Vlasov Simulation of Ion Acoustic Double Layers.- 1. Introduction.- 2. Description of “Vlasov” Code.- 3. The Formation of Ion Acoustic Double Layers.- References.- Simulation Models for Space Plasmas and Boundary Conditions as a Key to their Design and Analysis.- 1. Introduction.- 2. Simulation Models and Boundary Conditions Derived from Laboratory Plasmas.- 3. Simulation Models and Boundary Conditions Specific of Space Plasmas.- 4. Boundary Conditions and the Soluton of Field Equation.- 5. Boundary Conditions for Charged Particle.- 6. Coupling of Local and Global Dynamics.- References.