Atnaujinkite slapukų nuostatas

El. knyga: Plasmas and Energetic Processes in the Geomagnetosphere. Volume II: Plasmas/Magnetic and Current Sheets, Reconnections, Particle Acceleration, and Substorms

  • Formatas: 561 pages
  • Išleidimo metai: 01-Dec-2016
  • Leidėjas: Nova Science Publishers Inc
  • ISBN-13: 9781536101447
Kitos knygos pagal šią temą:
  • Formatas: 561 pages
  • Išleidimo metai: 01-Dec-2016
  • Leidėjas: Nova Science Publishers Inc
  • ISBN-13: 9781536101447
Kitos knygos pagal šią temą:

DRM apribojimai

  • Kopijuoti:

    neleidžiama

  • Spausdinti:

    neleidžiama

  • El. knygos naudojimas:

    Skaitmeninių teisių valdymas (DRM)
    Leidykla pateikė šią knygą šifruota forma, o tai reiškia, kad norint ją atrakinti ir perskaityti reikia įdiegti nemokamą programinę įrangą. Norint skaityti šią el. knygą, turite susikurti Adobe ID . Daugiau informacijos  čia. El. knygą galima atsisiųsti į 6 įrenginius (vienas vartotojas su tuo pačiu Adobe ID).

    Reikalinga programinė įranga
    Norint skaityti šią el. knygą mobiliajame įrenginyje (telefone ar planšetiniame kompiuteryje), turite įdiegti šią nemokamą programėlę: PocketBook Reader (iOS / Android)

    Norint skaityti šią el. knygą asmeniniame arba „Mac“ kompiuteryje, Jums reikalinga  Adobe Digital Editions “ (tai nemokama programa, specialiai sukurta el. knygoms. Tai nėra tas pats, kas „Adobe Reader“, kurią tikriausiai jau turite savo kompiuteryje.)

    Negalite skaityti šios el. knygos naudodami „Amazon Kindle“.

The importance and actuality of the geomagnetosphere's research are based on the following three factors:1. The geomagnetosphere is the nearest giant natural laboratory, where it is possible by multiple satellites and ground measurements to investigate in detail many different plasmas and energetic processes in space; these are caused by the interaction of high kinetic energy solar wind plasmas and their perturbations (Coronal Mass Ejections - CME, Interplanetary Shock Waves - ISW, Interplanetary Interaction Regions - IIR) frozen in Interplanetary Magnetic Fields (IMF) with the rotated main geomagnetic field. This interaction leads to a dynamic transformation in magnetic fields in the geomagnetosphere, generation and trapping of high energy particles (which are also called Magnetospheric Cosmic Rays - MCR), and generation of instabilities and electromagnetic radiations. These processes are in principle similar to processes in magnetospheres of other planets and their moons, in the atmosphere of the Sun and other stars, in interplanetary and in interstellar space, and in many different astrophysical objects. Put simply, this research is an important basis for fundamental space and astrophysical science.2. In modern times, technology, economics, navigation, television, internet, radio connections, military and all aspects of people's lives on our planet are strongly connected with the work of many satellites moving inside the geomagnetosphere. Different processes and MCR in the geomagnetosphere influence satellites often lead to satellite malfunctions and sometimes fully destroying them. The described research can be considered as a basis for developing methods of forecasting dangerous situations for satellites in different orbits, and to decrease the risk of satellite malfunction and loss.3. The interaction of CME, ISW, and IIR with the geomagnetosphere leads to the generation of big magnetic storms accompanied with Forbush decrease and precursory effects in Galactic Cosmic Ray (GCR) intensity. These magnetic storms are dangerous not only for satellites, but also on the Earth's surface for technology, radio connections, car accidents, and human health (e.g., increasing frequency of infarct myocardial and strokes). Investigations of magnetic storm causes can help to develop methods of their forecasting and decrease the level of magnetic storm hazards. Therefore, the other practical application of this research is connected with the problem of space weather influence on the technology, radio connections, navigation, transportation, and human health on Earth in regards to altitude and latitude. Target Audience:The authors hope that this book will be interesting and useful for researches, engineers, and students of corresponding specialties.
Preface xi
Acknowledgments xix
Abbreviations and Notations xxiii
Author Contact Information xxxix
Chapter 1 Magnetospheric Sheets: Main Properties, Structure, Expansion, and Particle Transport
1(72)
1.1 Main Properties of the Plasmas/Current/Magnetic Sheets
1(12)
1.2 Plasmas, Magnetic, and Current Sheets Thickness and Structure
13(17)
1.3 Plasmas and Magnetic Sheets Expansion, Magnetic Flux and Particle Acceleration/Transport
30(26)
1.4 Current Sheets Expansion, Magnetic Flux and Particle Transport
56(17)
References for
Chapter 1
63(10)
Chapter 2 Turbulence and Fluctuations, Instabilities, Storm Time Variations, Fast Flows, Temperature Anisotropies, and Magnetic Field Structure in Magnetospheric Sheets
73(88)
2.1 Turbulence and Fluctuations in the Magnetospheric Plasma Sheet
73(17)
2.2 Instabilities in the Plasma and Current Sheets
90(9)
2.3 Storm Time Plasma Sheet
99(7)
2.4 Earthward Fast Flows in the Plasma Sheet
106(21)
2.5 Electron and Ion Temperature Anisotropies and Asimmetries in the Geomagnetospheric Sheathes
127(4)
2.6 Magnetic Field in the Magnetosheath
131(30)
References for
Chapter 2
146(15)
Chapter 3 Magnetospheric Sheets: Bifurcation and Flapping, Pressure Gradients, Influence of Solar Wind and IMF Conditions, ULF, EUV, Auroral Arc Waves, Dipolarization and Antidipolarization Fronts, Parallel Electric Fields, Plasmoids and Jets
161(68)
3.1 Bifurcated Current Sheet and Flapping Motions
161(7)
3.2 Pressure Gradients in the Plasma Sheet
168(6)
3.3 Influence of Solar Wind and IMF Conditions, as Well as Geomagnetic Activity on Plasma Sheet
174(14)
3.4 ULF, EUV, Auroral Arc Waves, and Other Waves in the Plasma/Magneto Sheaths
188(4)
3.5 Aurora and Plasma Sheet Dynamics
192(2)
3.6 Interaction between Terrestrial Plasma Sheet and the Lunar Surface
194(1)
3.7 Dipolarization and Antidipolarization Fronts in the Magnetotail Plasma Sheet
195(4)
3.8 Parallel Electric Fields, Entropy Distribution, and Ionospheric Cold Ions in Plasma Sheet
199(2)
3.9 Plasmoids and Jets in Magnetosheath
201(1)
3.10 Properties and Processes in the Current Sheets
202(27)
References for
Chapter 3
218(11)
Chapter 4 Main Properties, Onset and Expansion Phases of Substorms
229(70)
4.1 Main Properties of Substorms
229(5)
4.2 Onset and Expansion Phase of Substorms
234(11)
4.3 Events Near Substorm Onset
245(2)
4.4 Models and Simulations for Substorm Expansion Phase Onset
247(4)
4.5 Substorms in the Earth's Tail and Plasma Sheet
251(11)
4.6 Substorm Trigger Processes
262(6)
4.7 Observations of Individual Substorms
268(3)
4.8 Location of the Substorm Onset
271(2)
4.9 Relationship between the Conditions in the Interplanetary Space and the Substorm Expansion Phase
273(5)
4.10 Substorm Breakup and Pseudobreakup
278(1)
4.11 Substorms and auroras
279(5)
4.12 Subauroral Polarization Stream Intensification during Substorms
284(1)
4.13 Measurements of the Substorm Current Wedge
285(14)
References for
Chapter 4
286(13)
Chapter 5 Substorms: Reconnections, Particle Acceleration, and Statistical Studies
299(88)
5.1 Reconnection, Convection, Turbulence, and Magnetospheric Disruptions
299(6)
5.2 Phenomena Induced Magnetic Reconnection
305(2)
5.3 Phenomena Accompanied Magnetic Reconnection
307(23)
5.4 Particle Acceleration during Reconnection
330(4)
5.5 Observations of Magnetic Reconnections
334(4)
5.6 Reconnection Rate, FTEs and NFTEs
338(4)
5.7 THEMIS Substorm Events Implying Magnetic Reconnection as the Substorm Trigger
342(1)
5.8 Magnetic Reconnection and Kelvin-Helmholtz Instabilities
343(1)
5.9 Magnetic Reconnection and Tearing Instability, Turbulence, Asymmetry, Power Density, Gyrotropy, Electron Pressure Anisotropy, Field-Aligned Currents, Alfvenic Resonance Layers
344(8)
5.10 Collisionless and Spontaneous Magnetic Reconnections, Exhaust Jets
352(3)
5.11 Statistical Studies of Open Magnetic Flux And Energy Release at Substorm Onset
355(1)
5.12 Statistical Studies of Isolated and Non- Isolated Substorms
356(5)
5.13 Relation between Solar Wind/IMF and Substorm Dynamics
361(1)
5.14 Magnetotail Flux Transport and Magnetotail Activity during Substorms
362(2)
5.15 Statistical Studies of Magnetospheric Substorms and PC Index, Using Ground-Based Magnetometer Stations, Growth and Spatial Scales of the Substorm Onset Arc
364(2)
5.16 Investigations of Magnetic Reconnection in the Boundary Regions of the Geomagnetosphere (Particularly Along Its Dayside Boundary with the Solar Wind and the Neutral Sheet in Magnetotail)
366(21)
References for
Chapter 5
372(15)
Chapter 6 Modeling and Simulation of Magnetospheric Substorms and Related Phenomena
387(66)
6.1 Multiscale and Multifractal Models
387(4)
6.2 MHD and Global Particle Simulations
391(10)
6.3 NECM Model
401(1)
6.4 Substorms as Nonequilibrium Magnetosphere Transitions
402(1)
6.5 Models with Anisotropic Pressure
402(3)
6.6 Spontaneous Fast and Steady-State Reconnection Models
405(3)
6.7 Asymmetric Reconnection
408(1)
6.8 Coupling of Charged Particles via Coulombic Interactions
409(1)
6.9 Modeling a Force-Free FTE during Substorms and Rice Convection Model
410(2)
6.10 Outside--in and inside--out Scenarios; Nonlinear Dynamical Bifurcation Model
412(1)
6.11 Mechanism of Substorm Current Wedge Formation
412(2)
6.12 State Space Model and Advances in Understanding Substorm Dynamics
414(1)
6.13 Substorms: Pre-Onset Arc, as response to IMF Discontinuities, Modeling Spontaneous Reconnection, Birkeland Currents, and Westward Traveling Surge
415(2)
6.14 Substorms and Auroral Phenomena
417(15)
6.15 Multiscale Phenomena Associated with Substorms
432(2)
6.16 Substorms and Magnetic Field Dipolarizations
434(9)
6.17 Formation of Downstream High-Speed Jets
443(10)
References for
Chapter 6
444(9)
Chapter 7 Substorms Energetics, Relation with Magnetic Storms, Pulsations, Turbulence, Plasma Bubbles, Substorm Index, and Jets
453(40)
7.1 Substorms and Geomagnetosphere Energetics
453(6)
7.2 Relation between Substorms and Magnetic Storms
459(3)
7.3 Energetic Neutral Atoms (ENAs) during Substorms
462(1)
7.4 Energetic Charged Particles during Substorms
463(10)
7.5 Substorms and Plasmas-Energetic Processes in the Ionosphere
473(6)
7.6 Substorms and Magnetic Activity, Pulsations, Turbulence, Plasma Bubbles, New Substorm Index, Space Climate, CR Asymptotic Directions, X-Ray Emission, Polarization Jet and Injection Boundary of Energetic Ions
479(14)
References for
Chapter 7
486(7)
References for Monographs and Books 493(10)
Object Index 503(10)
Author Index 513