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- English
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Multiscale Coupling of Sun-Earth Processes
About This Book
Many approaches exist for scientific investigations and space research is no exception. The early approach during which each space plasma region within the Sun-Earth system was investigated separately with physics-based tools has now progressed to encompass investigations on coupling between these regions. Ample evidence now exists indicating the dynamic processes in these regions exhibit disturbances over a wide range of scales both in time and space. This new reckoning naturally leads to an emerging perspective of probing these natural phenomena with concepts and tools developed in modern statistical mechanics for physical processes governing the evolution of out-of-equilibrium and complex systems.
These new developments have prompted a topical conference on Sun-Earth connection, held on February 9-13, 2004 at Kailua-Kona, Hawaii, USA, with the goal of promoting interactions among scientists practicing the traditional physics-based approach and those utilizing modern statistical techniques.
This monograph is a product of this conference, a compilation of thirty-nine articles assembled into seven chapters: (1) multiscale features in complexity dynamics, (2) space storms, (3) magnetospheric substorms, (4) turbulence and magnetic reconnection, (5) modeling and coupling of space phenomena, (6) techniques for multiscale space plasma problems, and (7) present and future multiscale space missions. These articles show a diversity of space phenomena exhibiting scale free characteristics, intermittency, and non-Gaussian distributions of probability density function of fluctuations in the physical parameters of the Sun-Earth system. The scope covers the latest observations, theories, simulations, and techniques on the multiscale nature of Sun-Earth phenomena and underscores the usefulness in cross-disciplinary exchange needed to unravel the underlying physical processes, which may eventually lead to a possible unified description and prediction for space disturbances.* Extensive collection of state-of-the-art papers on multiscale coupling of Sun-Earth Processes
* Present and future multiscale space missions
* New techniques and models for performing multiscale analysis
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Table of contents
- Cover image
- Title page
- Table of Contents
- Copyright
- PREFACE
- Chapter 1: COMPLEXITY IN SPACE PLASMAS
- Chapter 2: INTERMITTENCY IN SPACE PLASMA TURBULENCE
- Chapter 3: SCALE-DEPENDENT ANISOTROPY OF MAGNETIC FLUCTUATIONS IN THE EARTH’S PLASMA SHEET
- Chapter 4: HOW DOES THE SOLAR WIND POWER THE MAGNETOSPHERE DURING GEO-EFFECTIVE HIGH SPEED STREAMS?
- Chapter 5: ON THE IDENTIFICATION OF SOC DYNAMICS IN THE SUN-EARTH SYSTEM
- Chapter 6: LONG-STANDING UNSOLVED PROBLEMS IN SOLAR PHYSICS AND MAGNETOSPHERIC PHYSICS
- Chapter 7: SPACE WEATHER EFFECTS ON SOHO AND ITS LEADING ROLE AS A SPACE WEATHER WATCHDOG
- Chapter 8: STATISTICAL PRECURSORS TO SPACE STORM ONSET
- Chapter 9: SOLAR WIND DRIVERS FOR STEADY MAGNETOSPHERIC CONVECTION
- Chapter 10: GEOEFFECTIVENESS OF SHOCKS IN POPULATING THE RADIATION BELTS
- Chapter 11: COUPLING OF RELATIVISTIC ELECTRONS IN THE INNER MAGNETOSPHERE TO SPACE WEATHER PHENOMENA
- Chapter 12: THE LOWEST POSSIBLE LATITUDE OF THE WESTWARD ELECTROJET DURING SEVERELY DISTURBED PERIODS
- Chapter 13: GLOBAL DAYSIDE IONOSPHERIC RESPONSE TO INTERPLANETARY ELECTRIC FIELDS: PLASMA UPLIFT AND INCREASES IN TOTAL ELECTRON CONTENT
- Chapter 14: WHAT DETERMINES THE INTENSITY OF MAGNETOSPHERIC SUBSTORMS?
- Chapter 15: ROLES OF CHAOS, SELF-ORGANIZED CRITICALITY AND PHASE TRANSITIONS IN MAGNETOSPHERIC PHYSICS
- Chapter 16: SUBSTORM ONSET CAUSED BY THE TWO STATE TRANSITION OF THE MAGNETOSPHERE
- Chapter 17: EXPLOSIVE INSTABILITIES AND SUBSTORM INTENSIFICATIONS IN THE EARTH’S MAGNETOTAIL
- Chapter 18: SUBSTORM AURORAL MORPHOLOGY DURING GEOMAGNETIC STORMS ON 19-20 APRIL 2002
- Chapter 19: PERIODIC SUBSTORMS: A NEW PERIODICITY OF 2-3 HOURS IN THE MAGNETOSPHERE
- Chapter 20: MAGNETIC FIELD FLUCTUATIONS IN THE PLASMA SHEET REGION: A STATISTICAL APPROACH
- Chapter 21: NUMERICAL SIMULATIONS OF SOLAR WIND TURBULENCE
- Chapter 22: INTERMITTENT TURBULENCE IN 2D MHD SIMULATION
- Chapter 23: INTERMITTENCY AND SELF-SIMILARITY IN ‘NATURAL PARAMETERS’ IN SOLAR WIND TURBULENCE
- Chapter 24: ACCELERATION OF PARTICLES BY LOWER-HYBRID WAVES IN SPACE PLASMAS
- Chapter 25: SUBSTORM DISTURBANCE PROPAGATION FROM A TWO-DIMENSIONAL CELLULAR AUTOMATON MODEL
- Chapter 26: A Perspective of E+VxB=0 from the Special Theory of Relativity
- Chapter 27: ENERGIZATION OF IONS BY BIMODAL INTERMITTENT FLUCTUATIONS
- Chapter 28: A PHYSICS-BASED SOFTWARE FRAMEWORK FOR SUN-EARTH CONNECTION MODELING
- Chapter 29: A COMPARATIVE STUDY OF PROBABILITY DISTRIBUTION FUNCTIONS AND BURST LIFETIME DISTRIBUTIONS OF BS AND AE AT SOLAR MAXIMUM AND MINIMUM
- Chapter 30: THE DAYTIME CUSP AURORA IN THE O(1D) EMISSION OBSERVED BY WINDII ON UARS
- Chapter 31: THE WAVELENGTH OF SLOW MHD WAVES OBSERVED IN THE NIGHT-SIDE PLASMA SHEET
- Chapter 32: WINDMI: A FAMILY OF PHYSICS NETWORK MODELS FOR STORMS AND SUBSTORMS
- Chapter 33: A THREE-FLUID MODEL OF SOLAR WIND-MAGNETOSPHERE-IONOSPHERE-THERMOSPHERE COUPLING
- Chapter 34: 3D PLASMA STRUCTURES OBSERVED BY THE FOUR CLUSTER SPACECRAFT
- Chapter 35: THE CENTRAL ROLE OF RECONNECTION IN SPACE PLASMA PHENOMENA TARGETED BY THE MAGNETOSPHERIC MULTISCALE MISSION
- Chapter 36: MULTISCALE GEOSPACE PHYSICS IN CANADA
- Chapter 37: A CHINESE-EUROPEAN MULTISCALE MISSION: THE DOUBLE STAR PROGRAM
- Author Index