Magnetohydrodynamic Modeling Of The Solar Corona And Heliosphere
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Magnetohydrodynamic Modeling Of The Solar Corona And Heliosphere
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Author : Xueshang Feng
language : en
Publisher: Springer
Release Date : 2019-08-01
Magnetohydrodynamic Modeling Of The Solar Corona And Heliosphere written by Xueshang Feng and has been published by Springer this book supported file pdf, txt, epub, kindle and other format this book has been release on 2019-08-01 with Science categories.
The book covers intimately all the topics necessary for the development of a robust magnetohydrodynamic (MHD) code within the framework of the cell-centered finite volume method (FVM) and its applications in space weather study. First, it presents a brief review of existing MHD models in studying solar corona and the heliosphere. Then it introduces the cell-centered FVM in three-dimensional computational domain. Finally, the book presents some applications of FVM to the MHD codes on spherical coordinates in various research fields of space weather, focusing on the development of the 3D Solar-InterPlanetary space-time Conservation Element and Solution Element (SIP-CESE) MHD model and its applications to space weather studies in various aspects. The book is written for senior undergraduates, graduate students, lecturers, engineers and researchers in solar-terrestrial physics, space weather theory, modeling, and prediction, computational fluid dynamics, and MHD simulations. It helps readers to fully understand and implement a robust and versatile MHD code based on the cell-centered FVM.
Magnetohydrodynamic Modeling Of The Solar Corona And Heliosphere
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Author : Xueshang Feng
language : en
Publisher:
Release Date : 2020
Magnetohydrodynamic Modeling Of The Solar Corona And Heliosphere written by Xueshang Feng and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 2020 with Heliosphere (Astrophysics) categories.
The book covers intimately all the topics necessary for the development of a robust magnetohydrodynamic (MHD) code within the framework of the cell-centered finite volume method (FVM) and its applications in space weather study. First, it presents a brief review of existing MHD models in studying solar corona and the heliosphere. Then it introduces the cell-centered FVM in three-dimensional computational domain. Finally, the book presents some applications of FVM to the MHD codes on spherical coordinates in various research fields of space weather, focusing on the development of the 3D Solar-InterPlanetary space-time Conservation Element and Solution Element (SIP-CESE) MHD model and its applications to space weather studies in various aspects. The book is written for senior undergraduates, graduate students, lecturers, engineers and researchers in solar-terrestrial physics, space weather theory, modeling, and prediction, computational fluid dynamics, and MHD simulations. It helps readers to fully understand and implement a robust and versatile MHD code based on the cell-centered FVM.
Magnetohydrodynamics Of The Sun
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Author : Eric Priest
language : en
Publisher: Cambridge University Press
Release Date : 2014-04-07
Magnetohydrodynamics Of The Sun written by Eric Priest and has been published by Cambridge University Press this book supported file pdf, txt, epub, kindle and other format this book has been release on 2014-04-07 with Science categories.
This advanced textbook reviews the complex interaction between the Sun's plasma atmosphere and its magnetic field.
Advanced Magnetohydrodynamics
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Author : J. P. Goedbloed
language : en
Publisher: Cambridge University Press
Release Date : 2010-04-29
Advanced Magnetohydrodynamics written by J. P. Goedbloed and has been published by Cambridge University Press this book supported file pdf, txt, epub, kindle and other format this book has been release on 2010-04-29 with Science categories.
Following on from the companion volume Principles of Magnetohydrodynamics, this textbook analyzes the applications of plasma physics to thermonuclear fusion and plasma astrophysics from the single viewpoint of MHD. This approach turns out to be ever more powerful when applied to streaming plasmas (the vast majority of visible matter in the Universe), toroidal plasmas (the most promising approach to fusion energy), and nonlinear dynamics (where it all comes together with modern computational techniques and extreme transonic and relativistic plasma flows). The textbook interweaves theory and explicit calculations of waves and instabilities of streaming plasmas in complex magnetic geometries. It is ideally suited to advanced undergraduate and graduate courses in plasma physics and astrophysics.
Magnetohydrodynamics
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Author : J. P. Goedbloed
language : en
Publisher: Cambridge University Press
Release Date : 2019-01-31
Magnetohydrodynamics written by J. P. Goedbloed and has been published by Cambridge University Press this book supported file pdf, txt, epub, kindle and other format this book has been release on 2019-01-31 with Science categories.
An introduction to magnetohydrodynamics combining theory with advanced topics including the applications of plasma physics to thermonuclear fusion and plasma astrophysics.
A Three Dimensional Adaptive Multifluid Mhd Model Of The Heliosphere
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Author : Timur Jaan Linde
language : en
Publisher:
Release Date : 1998
A Three Dimensional Adaptive Multifluid Mhd Model Of The Heliosphere written by Timur Jaan Linde and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1998 with Heliosphere (Astrophysics) categories.
New Millennium Solar Physics
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Author : Markus J. Aschwanden
language : en
Publisher: Springer
Release Date : 2019-05-22
New Millennium Solar Physics written by Markus J. Aschwanden and has been published by Springer this book supported file pdf, txt, epub, kindle and other format this book has been release on 2019-05-22 with Science categories.
This is a follow-on book to the introductory textbook "Physics of the Solar Corona" previously published in 2004 by the same author, which provided a systematic introduction and covered mostly scientific results from the pre-2000 era. Using a similar structure as the previous book the second volume provides a seamless continuation of numerous novel research results in solar physics that emerged in the new millennium (after 2000) from the new solar missions of RHESSI, STEREO, Hinode, CORONAS, and the Solar Dynamics Observatory (SDO) during the era of 2000-2018. The new solar space missions are characterized by unprecedented high-resolution imaging, time resolution, spectral capabilities, stereoscopy and tomography, which reveal the intricate dynamics of magneto-hydrodynamic processes in the solar corona down to scales of 100 km. The enormous amount of data streaming down from SDO in Terabytes per day requires advanced automated data processing methods. The book focuses exclusively onnew research results after 2000, which are reviewed in a comprehensive manner, documented by over 3600 literature references, covering theory, observations, and numerical modeling of basic physical processes that are observed in high-temperature plasmas of the Sun and other astrophysical objects, such as plasma instabilities, coronal heating, magnetic reconnection processes, coronal mass ejections, plasma waves and oscillations, or particle acceleration.
Low Frequency Waves In Space Plasmas
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Author : Andreas Keiling
language : en
Publisher: John Wiley & Sons
Release Date : 2016-04-04
Low Frequency Waves In Space Plasmas written by Andreas Keiling and has been published by John Wiley & Sons this book supported file pdf, txt, epub, kindle and other format this book has been release on 2016-04-04 with Science categories.
Low-frequency waves in space plasmas have been studied for several decades, and our knowledge gain has been incremental with several paradigm-changing leaps forward. In our solar system, such waves occur in the ionospheres and magnetospheres of planets, and around our Moon. They occur in the solar wind, and more recently, they have been confirmed in the Sun’s atmosphere as well. The goal of wave research is to understand their generation, their propagation, and their interaction with the surrounding plasma. Low-frequency Waves in Space Plasmas presents a concise and authoritative up-to-date look on where wave research stands: What have we learned in the last decade? What are unanswered questions? While in the past waves in different astrophysical plasmas have been largely treated in separate books, the unique feature of this monograph is that it covers waves in many plasma regions, including: Waves in geospace, including ionosphere and magnetosphere Waves in planetary magnetospheres Waves at the Moon Waves in the solar wind Waves in the solar atmosphere Because of the breadth of topics covered, this volume should appeal to a broad community of space scientists and students, and it should also be of interest to astronomers/astrophysicists who are studying space plasmas beyond our Solar System.
Collisionless Shocks In The Heliosphere
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Author : Robert G. Stone
language : en
Publisher: American Geophysical Union
Release Date : 1985
Collisionless Shocks In The Heliosphere written by Robert G. Stone and has been published by American Geophysical Union this book supported file pdf, txt, epub, kindle and other format this book has been release on 1985 with Science categories.
Published by the American Geophysical Union as part of the Geophysical Monograph Series, Volume 35. Violent expansions of the solar corona cause transient shock waves which propagate outward from the sun at hundreds to thousands of kilometers per second; simple solar wind velocity gradients at the surface of the sun lead to high-speed streams overtaking slower streams, forming corotating shocks; and steady state supermagnetosonic solar wind flow past objects such as the planets lead to standing bow shocks. However, the solar wind plasma is so hot and tenuous that charged particle Coulomb collisions produce negligible thermalization or dissipation on scale sizes less than 0.1 AU. The irreversible plasma heating by these shocks is accomplished by wave-particle interactions driven by plasma instabilities. Hence these shocks are described as "collisionless."
Reviews In Astronomy And Space Sciences
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Author : Christopher H. K. Chen
language : en
Publisher: Frontiers Media SA
Release Date : 2024-05-24
Reviews In Astronomy And Space Sciences written by Christopher H. K. Chen and has been published by Frontiers Media SA this book supported file pdf, txt, epub, kindle and other format this book has been release on 2024-05-24 with Science categories.