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Waves, Particles, and Storms in Geospace, 1. udgave

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Georgios Balasis, Ioannis A. Daglis og I. R. Mann
(2016)
Oxford University Press
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Waves, Particles, and Storms in Geospace, 1. udgave

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(2016)
Oxford University Press
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Georgios Balasis, Ioannis A. Daglis og I. R. Mann
(2016)
Oxford University Press
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Waves, Particles, and Storms in Geospace - A Complex Interplay

Waves, Particles, and Storms in Geospace

A Complex Interplay
Georgios Balasis, Ioannis A. Daglis og Ian R. Mann
(2017)
Sprog: Engelsk
Oxford University Press, Incorporated
1.677,00 kr.
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  • 1. Udgave
  • Vital Source 180 day rentals (fixed pages)
  • Udgiver: Oxford University Press (November 2016)
  • Forfattere: Georgios Balasis, Ioannis A. Daglis og I. R. Mann
  • ISBN: 9780191015359R180
Geospace features highly dynamic populations of charged particles with a wide range of energies from thermal to ultra-relativistic. Influenced by magnetic and electric fields in the terrestrial magnetosphere driven by solar wind forcing, changes in the numbers and energies of these particles lead to a variety of space weather phenomena, some of which are detrimental to space infrastructure. This book presents an overview of the latest discoveries and current scientific understanding of the coupling of electromagnetic waves and charged particles during magnetic storms, and explains the observed dynamics of these particle populations. The book furthermore includes investigations relevant to understanding and forecasting this space environment and the adverse impacts of space weather. High-energy electrons and ions in the Van Allen radiation belts and the ring current are of particular interest and importance with regard to the operation of space-based technological infrastructure upon which 21st century civilisation increasingly relies. This book presents the latest research on the sources, transport, acceleration and loss of these energetic particle populations, as well as their coupling during geospace magnetic storms.
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Detaljer om varen

  • 1. Udgave
  • Vital Source 365 day rentals (fixed pages)
  • Udgiver: Oxford University Press (November 2016)
  • ISBN: 9780191015359R365
Geospace features highly dynamic populations of charged particles with a wide range of energies from thermal to ultra-relativistic. Influenced by magnetic and electric fields in the terrestrial magnetosphere driven by solar wind forcing, changes in the numbers and energies of these particles lead to a variety of space weather phenomena, some of which are detrimental to space infrastructure. This book presents an overview of the latest discoveries and current scientific understanding of the coupling of electromagnetic waves and charged particles during magnetic storms, and explains the observed dynamics of these particle populations. The book furthermore includes investigations relevant to understanding and forecasting this space environment and the adverse impacts of space weather. High-energy electrons and ions in the Van Allen radiation belts and the ring current are of particular interest and importance with regard to the operation of space-based technological infrastructure upon which 21st century civilisation increasingly relies. This book presents the latest research on the sources, transport, acceleration and loss of these energetic particle populations, as well as their coupling during geospace magnetic storms.
Licens varighed:
Online udgaven er tilgængelig: 365 dage fra købsdato.
Offline udgaven er tilgængelig: 365 dage fra købsdato.

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  • 1. Udgave
  • Vital Source 1460 day rentals (fixed pages)
  • Udgiver: Oxford University Press (November 2016)
  • ISBN: 9780191015359R1460
Geospace features highly dynamic populations of charged particles with a wide range of energies from thermal to ultra-relativistic. Influenced by magnetic and electric fields in the terrestrial magnetosphere driven by solar wind forcing, changes in the numbers and energies of these particles lead to a variety of space weather phenomena, some of which are detrimental to space infrastructure. This book presents an overview of the latest discoveries and current scientific understanding of the coupling of electromagnetic waves and charged particles during magnetic storms, and explains the observed dynamics of these particle populations. The book furthermore includes investigations relevant to understanding and forecasting this space environment and the adverse impacts of space weather. High-energy electrons and ions in the Van Allen radiation belts and the ring current are of particular interest and importance with regard to the operation of space-based technological infrastructure upon which 21st century civilisation increasingly relies. This book presents the latest research on the sources, transport, acceleration and loss of these energetic particle populations, as well as their coupling during geospace magnetic storms.
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Detaljer om varen

  • 1. Udgave
  • Vital Source searchable e-book (Fixed pages)
  • Udgiver: Oxford University Press (November 2016)
  • Forfattere: Georgios Balasis, Ioannis A. Daglis og I. R. Mann
  • ISBN: 9780191015359
Geospace features highly dynamic populations of charged particles with a wide range of energies from thermal to ultra-relativistic. Influenced by magnetic and electric fields in the terrestrial magnetosphere driven by solar wind forcing, changes in the numbers and energies of these particles lead to a variety of space weather phenomena, some of which are detrimental to space infrastructure. This book presents an overview of the latest discoveries and current scientific understanding of the coupling of electromagnetic waves and charged particles during magnetic storms, and explains the observed dynamics of these particle populations. The book furthermore includes investigations relevant to understanding and forecasting this space environment and the adverse impacts of space weather. High-energy electrons and ions in the Van Allen radiation belts and the ring current are of particular interest and importance with regard to the operation of space-based technological infrastructure upon which 21st century civilisation increasingly relies. This book presents the latest research on the sources, transport, acceleration and loss of these energetic particle populations, as well as their coupling during geospace magnetic storms.
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Online udgaven er tilgængelig: 365 dage fra købsdato.
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Detaljer om varen

  • Hardback: 320 sider
  • Udgiver: Oxford University Press, Incorporated (Januar 2017)
  • Forfattere: Georgios Balasis, Ioannis A. Daglis og Ian R. Mann
  • ISBN: 9780198705246
Geospace features highly dynamic populations of charged particles with a wide range of energies from thermal to ultra-relativistic. Influenced by magnetic and electric fields in the terrestrial magnetosphere driven by solar wind forcing, changes in the numbers and energies of these particles lead to a variety of space weather phenomena, some of which are detrimental to space infrastructure. This book presents an overview of the latest discoveries and current scientific understanding of the coupling of electromagnetic waves and charged particles during magnetic storms, and explains the observed dynamics of these particle populations. The book furthermore includes investigations relevant to understanding and forecasting this space environment and the adverse impacts of space weather.

High-energy electrons and ions in the Van Allen radiation belts and the ring current are of particular interest and importance with regard to the operation of space-based technological infrastructure upon which 21st century civilisation increasingly relies. This book presents the latest research on the sources, transport, acceleration and loss of these energetic particle populations, as well as their coupling during geospace magnetic storms.

Waves, Particles, and Storms in Geospace: An Introduction Ian R. Mann Geospace storms and radiation belt dynamics A new era of radiation belt research Wave-particle interactions and their impacts on the radiation belts Coupling between the radiation belts and the neutral atmosphere: potential impact on climate Space plasma physics in the heliosphere Applied heliophysics research: space weather Conclusions and future perspective References Preface 1 Wave and Particle Measurements in Earth''s Neighborhood: A Historical Mission Overview D. N. Baker
1.1 Introduction
1.2 1950s: A new dawn -- The "Space Age"
1.3 1960s: Our place in space -- morphology and plasma domains
1.4 1970s: System dynamics -- storms and substorms
1.5 1980s: Universal processes -- reconnection and acceleration
1.6 1990s: Follow the energy -- solar-terrestrial coupling
1.7 2000s: Multiscale phenomena -- the telescope-microscope duality
1.8 2010s: The Sun-Earth system -- space weather and beyond References 2 Introduction to Wave-Particle Interactions and their Impact on Energetic Particles in Geospace Kazue Takahashi and Yoshizumi Miyoshi
2.1 Introduction
2.2 Impact of wave-particle interaction on electron acceleration and loss
2.3 General observational approach to wave-particle interactions
2.4 Experimental resources
2.5 Example of observational studies of waves and particles
2.5.1 ULF wave-particle interaction
2.5.2 Two-spacecraft measurements of wave propagation
2.5.3 Ground-satellite observation of EMIC waves, aurora, and particle precipitation
2.5.4 Nonlinear wave-particle interactions
2.6 Summary Acknowledgments References 3 Geospace Magnetic Storms and the Van Allen Radiation Belts Geoffrey D. Reeves and Ioannis A. Daglis
3.1 Introduction
3.2 Electron motion in Earth''s radiation belts
3.3 Effects of geospace magnetic storms on the radiation belts
3.4 Local acceleration and radial diffusion
3.5 Phase space density gradients
3.6 Studies with the Van Allen Probes: insights into the effects of wave-particle interactions and the ring current influence
3.7 Summary Acknowledgments References 4 The Role of Pc-5 ULF Waves in the Radiation Belts: Current Understanding and Open Questions Scot R. Elkington and Theodore E. Sarris
4.1 The role of Pc-5 waves in the radiation belts
4.2 Questions: Quantitative determination of transport rates
4.2.1 What is the power spectrum as a function of frequency?
4.2.2 What is the radial profile of the ULF activity?
4.2.3 What is the azimuthal mode structure?
4.2.4 What is the azimuthal extent?
4.2.5 What is the propagation direction?
4.2.6 What is the origin of the waves?
4.3 Conclusions and future possibilities Acknowledgments References 5 Modeling the Energetic Particles of the Inner Magnetosphere S. Bourdarie, V. K. Jordanova, M. Liemohn, and T. P. O''Brien
5.1 Background
5.1.1 Trapped particle transport theory
5.2 Modeling ring current particles
5.2.1 Kinetic ring current models
5.2.2 Self-consistent models
5.3 Modeling radiation belt particles
5.3.1 3D diffusion model
5.3.2 Radiation specification models Acknowledgments References 6 Monitoring ULF Waves from Low Earth Orbit Satellites Georgios Balasis, Constantinos Papadimitriou, Eftyhia Zesta, and Viacheslav Pilipenko
6.1 Introduction
6.2 Methods and techniques
6.3 Studies of ULF wave observations from LEO
6.3.1 Pc1 wave observations
6.3.2 Pi1 bursts
6.3.3 Pc3 wave observations
6.3.4 Pi2 wave observations
6.3.5 Doppler effect on LEO observations
6.4 Modeling the relationship between the ULF compressional disturbance above the ionosphere and ground signal
6.5 Discussion: prospects of further studies Acknowledgments References 7 Monitoring Magnetospheric Waves from the Ground Colin Waters and Fred Menk
7.1 Overview of instrumentation and techniques
7.2 Remote sensing geospace using data from ground magnetometer arrays
7.2.1 Data analysis techniques
7.2.2 Remote sensing plasma mass density in space
7.3 Space weather applications
7.3.1 Remote sensing Pc5 electric fields
7.3.2 Latitude and local time dependence of Pc5 power
7.3.3 Storm-time Pc5 activity and indices
7.3.4 ULF Waves in the ionosphere
7.3.5 Favoured frequencies in the Pc5 band
7.3.6 Pc3 waves and indices
7.4 Summary Acknowledgments References 8 Chorus Waves in Geospace and their Influence on Radiation Belt Dynamics Jacob Bortnik, Richard M. Thorne, Wen Li, and Xin Tao
8.1 Introduction
8.2 Characteristics of chorus waves
8.3 Introduction to resonant wave particle interactions
8.4 Modes of interaction
8.4.1 Quasilinear diffusion
8.4.2 Nonlinear wave-particle interactions
8.5 Summary and conclusions References 9 Wave-Driven Diffusion in Radiation Belt Dynamics Richard B. Horne, Nigel P. Meredith, Sarah A. Glauert, and Tobias Kersten
9.1 Introduction
9.2 Magnetospheric plasma waves
9.2.1 Plasmaspheric hiss
9.2.2 Chorus
9.2.3 EMIC waves
9.2.4 Magnetosonic waves
9.3 Global simulations
9.3.1 Diffusion rates
9.3.2 Comparison with data
9.4 Discussion and conclusions Acknowledgments References 10 Understanding the Role of EMIC Waves in Radiation Belt and Ring Current Dynamics: Recent Advances Maria E. Usanova and Ian R. Mann
10.1 Introduction
10.2 EMIC wave excitation in the inner magnetosphere
10.2.1 Physical generation mechanisms for compression-related EMIC waves
10.2.2 Effect of solar wind dynamic pressure and enhanced cold plasma density on EMIC wave generation
10.2.3 Radial and MLT extent of EMIC waves
10.3 Role of EMIC waves in energetic particle loss
10.3.1 Role in ion precipitation into the atmosphere
10.3.2 Role in radiation belt electron precipitation
10.4 Discussion and conclusions Acknowledgments References 11 Multi-dimensional Analysis of Whistler-mode Waves in the Radiation Belt Region O. Santolík
11.1 Introduction
11.2 Analysis methods
11.2.1 Plane wave techniques
11.2.2 Wave distribution function
11.2.3 Instantaneous amplitude, phase, frequency, and wave vector direction
11.3 Examples of results
11.3.1 Plane wave techniques and wave distribution function methods for onboard-analyzed spectral data from the Cluster spacecraft
11.3.2 Example of waveform measurements from the Van Allen Probes EMFISIS instrument: plane wave techniques and instantaneous wave parameters
11.4 Conclusions Acknowledgments References 12 Extreme Variability of Relativistic Electrons in Earth''s Outer Radiation Belt: An Overview and Recent Revelations D. L. Turner and V. Angelopoulos
12.1 Introduction
12.2 Physical processes that can drive extreme outer belt variability
12.2.1 Sources
12.2.2 Losses
12.2.3 Transport
12.3 Recent multipoint observational examples of extreme outer belt variability
12.3.1 Outer belt enhancements
12.3.2 Outer belt depletions
12.3.3 Complex outer belt structures: remnant belts
12.4 Outstanding questions and topics for future work
12.4.1 Concerning sources
12.4.2 Concerning losses
12.4.3 Concerning transport
12.5 Conclusions Acknowledgments References 13 Flux Enhancement of Relativistic Electrons Associated with Substorms Y. Miyoshi, R. Kataoka, and Y. Ebihara
13.1 Introduction
13.2 Solar wind parameter dependencies
13.3 Physics behind the solar wind parameter dependencies
13.4 Role of continuous substorm activities in the cross-energy coupling process
13.5 Summary Acknowledgments References 14 Linkages Between the Radiation Belts, Polar Atmosphere and Climate: Electron Precipitation Through Wave Particle Interactions M. A. Clilverd, C. J. Rodger, M. E. Andersson, A. Seppälä, and P. T. Verronen
14.1 Introduction
14.2 Overview of coupling process
14.3 Waves driving precipitation
14.4 Variations in precipitation
14.5 Atmospheric impact of electron precipitation
14.5.1 Odd nitrogen
14.5.2 Odd Hydrogen
14.6 Linkages to polar surface climate
14.6.1 Influence on polar climate
14.6.2 Possible significance to regional weather variability Acknowledgments References 15 Energetic Particles and Waves in the Outer Planet Radiation Belts N. Krupp, E. Roussos, C. Paranicas, A. Sicard, G. Hospodarsky, and Y. Shprits
15.1 Introduction
15.2 Charged particles
15.2.1 Jupiter
15.2.2 Saturn
15.2.3 Modelling of charged particles in the Jovian and Kronian radiation belts
15.3 Plasma waves
15.3.1 Jupiter observations
15.3.2 Saturn observations
15.3.3 Modelling wave-particle interaction
15.4 Future missions to the outer planets Acknowledgments References 16 Fields and Waves Influencing Radiation Belt Dynamics -- Results from the Van Allen Probes Mission C. A. Kletzing
16.1 Introduction
16.2 Instrumentation
16.3 Van Allen Probes mission goals
16.4 Whistler mode waves
16.4.1 Chorus emissions
16.4.2 Plasmaspheric hiss
16.5 Low frequen
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