標(biāo)題: Titlebook: Basics of Plasma Astrophysics; Claudio Chiuderi,Marco Velli Textbook 2015 Springer-Verlag Italia S.r.l., part of Springer Nature 2015 Astr [打印本頁(yè)] 作者: 頌歌 時(shí)間: 2025-3-21 16:05
書(shū)目名稱Basics of Plasma Astrophysics影響因子(影響力)
書(shū)目名稱Basics of Plasma Astrophysics影響因子(影響力)學(xué)科排名
書(shū)目名稱Basics of Plasma Astrophysics網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱Basics of Plasma Astrophysics網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱Basics of Plasma Astrophysics被引頻次
書(shū)目名稱Basics of Plasma Astrophysics被引頻次學(xué)科排名
書(shū)目名稱Basics of Plasma Astrophysics年度引用
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書(shū)目名稱Basics of Plasma Astrophysics讀者反饋
書(shū)目名稱Basics of Plasma Astrophysics讀者反饋學(xué)科排名
作者: Epidural-Space 時(shí)間: 2025-3-21 23:38
2198-7882 l principles rather than specialized jargon.Up-to-date discu.This book is an introduction to contemporary plasma physics that discusses the most relevant recent advances in the field and covers a careful choice of applications to various branches of astrophysics and space science. The purpose of the作者: aristocracy 時(shí)間: 2025-3-22 04:24
Textbook 2015 of applications to various branches of astrophysics and space science. The purpose of the book is to allow the student to master the basic concepts of plasma physics and to bring him or her up to date in a number of relevant areas of current research. Topics covered include orbit theory, kinetic th作者: enflame 時(shí)間: 2025-3-22 05:47 作者: acclimate 時(shí)間: 2025-3-22 09:45 作者: DIS 時(shí)間: 2025-3-22 13:57 作者: 聲音刺耳 時(shí)間: 2025-3-22 20:12
An Introduction to Plasma Physics,iverse. Basic plasma features such as ionization degree and the condition of quasi-neutrality are discussed. A heuristic derivation of fundamental plasma parameters, such as plasma frequency and Debye length are given. Finally, the different possible approaches to the physical description of plasma 作者: 易于交談 時(shí)間: 2025-3-23 01:06 作者: 鉗子 時(shí)間: 2025-3-23 01:40 作者: averse 時(shí)間: 2025-3-23 08:33 作者: 偶像 時(shí)間: 2025-3-23 10:08 作者: Gingivitis 時(shí)間: 2025-3-23 16:31 作者: 注入 時(shí)間: 2025-3-23 20:00
Magnetic Reconnection,onary reconnection models of Sweet-Parker and Petschek are described before analyzing the resistive instabilities of current sheets and, in particular, the tearing mode. The chapter concludes with reconnection instabilities of thin sheets, or plasmoid instabilities, and the consequent general nonsta作者: RACE 時(shí)間: 2025-3-24 00:45 作者: 淺灘 時(shí)間: 2025-3-24 06:15
Build-Up of Magnetic Fields,tlined. The more formal approach of mean-field electrodynamic is also exposed. Simple solutions of the dynamo equations are discussed. Finally, the problem of the creation of magnetic fields in an unmagnetized plasma is briefly considered.作者: Generic-Drug 時(shí)間: 2025-3-24 09:34
Claudio Chiuderi,Marco VelliCovers a careful selection of applications of plasma physics to various branches of astrophysics and space science.Emphasis on basic physical principles rather than specialized jargon.Up-to-date discu作者: 無(wú)關(guān)緊要 時(shí)間: 2025-3-24 11:05
UNITEXT for Physicshttp://image.papertrans.cn/b/image/181276.jpg作者: 走路左晃右晃 時(shí)間: 2025-3-24 15:27
Basics of Plasma Astrophysics978-88-470-5280-2Series ISSN 2198-7882 Series E-ISSN 2198-7890 作者: DAMP 時(shí)間: 2025-3-24 20:22 作者: BANAL 時(shí)間: 2025-3-25 01:05
The Mechanism of High-,, Superconductivity,and followed by a discussion of the hierarchy of moment equations and the fluid closure problem. The Vlasov equation for collisionless plasmas is presented and Jeans’ theorem concerning its solution is proved.作者: Bernstein-test 時(shí)間: 2025-3-25 04:17
Fundamental Theories of Physicsample of the ideal, neutral gas to establish the procedure, a derivation of the two-fluid plasma equation is carried out in detail. Finally, the one-fluid plasma equations are derived and their meaning discussed, with particular emphasis on energy equation and Ohm’s law.作者: nascent 時(shí)間: 2025-3-25 09:20
Fundamental Theories of Physicsns, both ideal and resistive, is presented and their consequences analyzed, in particular in connection with the time evolution of magnetic fields. MHD equilibria are then described, both when magnetic forces are absent (force-free fields) and when they are present. Finally, the concept of perturbed equilibrium states is introduced.作者: 使腐爛 時(shí)間: 2025-3-25 12:23 作者: 皺痕 時(shí)間: 2025-3-25 16:04 作者: Apraxia 時(shí)間: 2025-3-25 23:04 作者: 同步信息 時(shí)間: 2025-3-26 02:24
The Mechanism of High-,, Superconductivity,tlined. The more formal approach of mean-field electrodynamic is also exposed. Simple solutions of the dynamo equations are discussed. Finally, the problem of the creation of magnetic fields in an unmagnetized plasma is briefly considered.作者: saphenous-vein 時(shí)間: 2025-3-26 07:17 作者: 注意 時(shí)間: 2025-3-26 09:07
Nonlinear Excitations: Solitons,Large amplitude waves, or shocks, are the subject of this chapter. Shocks in neutral gases are briefly reviewed. MHD shocks are then treated in detail while a brief discussion of collisionless shocks is presented in the final section.作者: 公司 時(shí)間: 2025-3-26 15:08
Particle Orbit Theory,In which particle motion in assigned electric and magnetic fields is discussed and studied in detail in a few representative cases. Fundamental concepts such as guiding center motion, particle drifts, magnetic moment, and adiabatic invariants are introduced, and a brief discussion of the mirror force and magnetic bottles is presented.作者: Omnipotent 時(shí)間: 2025-3-26 18:15
Shocks,Large amplitude waves, or shocks, are the subject of this chapter. Shocks in neutral gases are briefly reviewed. MHD shocks are then treated in detail while a brief discussion of collisionless shocks is presented in the final section.作者: ECG769 時(shí)間: 2025-3-27 00:02 作者: antidote 時(shí)間: 2025-3-27 03:21 作者: 放氣 時(shí)間: 2025-3-27 08:45 作者: 許可 時(shí)間: 2025-3-27 10:25 作者: 空洞 時(shí)間: 2025-3-27 17:33 作者: 防水 時(shí)間: 2025-3-27 18:08
Magnetic Reconnection,onary reconnection models of Sweet-Parker and Petschek are described before analyzing the resistive instabilities of current sheets and, in particular, the tearing mode. The chapter concludes with reconnection instabilities of thin sheets, or plasmoid instabilities, and the consequent general nonstationary behavior of reconnection processes.作者: 適宜 時(shí)間: 2025-3-28 01:27
MHD Turbulence,e is presented and the fundamental results of Kolmogorov deduced. Their generalization to plasmas in the MHD regime is then discussed. The relevance of turbulence theory for the problem of solar coronal heating is the subject of the last section.作者: Multiple 時(shí)間: 2025-3-28 03:21
Build-Up of Magnetic Fields,tlined. The more formal approach of mean-field electrodynamic is also exposed. Simple solutions of the dynamo equations are discussed. Finally, the problem of the creation of magnetic fields in an unmagnetized plasma is briefly considered.作者: 奴才 時(shí)間: 2025-3-28 09:47 作者: extrovert 時(shí)間: 2025-3-28 14:12 作者: Notify 時(shí)間: 2025-3-28 16:13
Fundamental Theories of Physicsiverse. Basic plasma features such as ionization degree and the condition of quasi-neutrality are discussed. A heuristic derivation of fundamental plasma parameters, such as plasma frequency and Debye length are given. Finally, the different possible approaches to the physical description of plasma 作者: Cantankerous 時(shí)間: 2025-3-28 20:05 作者: ascend 時(shí)間: 2025-3-29 00:49 作者: Decline 時(shí)間: 2025-3-29 04:21 作者: hurricane 時(shí)間: 2025-3-29 11:16
The Mechanism of High-,, Superconductivity, geometry when gravity is present, including the well-known Rayleigh-Taylor and Kelvin-Helmholtz instabilities, and discuss the stabilizing effects of magnetic fields in these cases. The instabilities stemming from the combined effects of currents, current gradients, and pressure in the ideal plasma作者: 飛來(lái)飛去真休 時(shí)間: 2025-3-29 13:50
The Mechanism of High-,, Superconductivity,frequency effects leading to kinetic corrections are then discussed before introducing waves in completely kinetic regimes, where the phenomenon of Landau damping for ion-acoustic modes is treated in detail.作者: Hdl348 時(shí)間: 2025-3-29 19:08 作者: TEM 時(shí)間: 2025-3-29 22:38
Fundamental Theories of Physicse is presented and the fundamental results of Kolmogorov deduced. Their generalization to plasmas in the MHD regime is then discussed. The relevance of turbulence theory for the problem of solar coronal heating is the subject of the last section.作者: Alpha-Cells 時(shí)間: 2025-3-30 01:07
The Mechanism of High-,, Superconductivity,tlined. The more formal approach of mean-field electrodynamic is also exposed. Simple solutions of the dynamo equations are discussed. Finally, the problem of the creation of magnetic fields in an unmagnetized plasma is briefly considered.
