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Energy transfer. --- Interplanetary magnetic fields. --- Magnetohydrodynamic flow. --- Magnetopause. --- Plasma sheaths. --- Solar wind.

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Despite the plethora of monographs published in recent years, few cover recent progress in magnetospheric physics in broad areas of research. While a topical focus is important to in-depth views at a problem, a broad overview of our field is also needed. The volume answers to the latter need. With the collection of articles written by leading scientists, the contributions contained in the book describe latest research results in solar wind-magnetosphere interaction, magnetospheric substorms, magnetosphere-ionosphere coupling, transport phenomena in the plasma sheet, wave and particle dynamics in the ring current and radiation belts, and extra-terrestrial magnetospheric systems. In addition to its breadth and timeliness, the book highlights innovative methods and techniques to study the geospace. Audience: This book is a handy reference for established scientists and an ideal guide for graduate students in the fields of geophysics, solar-terrestrial and magnetospheric physics.

Geophysics. --- Magnetopause. --- Magnetosphere. --- Polar cusp. --- Solar wind. --- Magnetosphere --- Physics --- Physical Sciences & Mathematics --- Cosmic Physics --- Earth sciences. --- Space sciences. --- Earth Sciences. --- Geophysics/Geodesy. --- Extraterrestrial Physics, Space Sciences. --- Atmosphere, Upper --- Upper atmosphere --- Physical geography. --- Astrophysics. --- Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). --- Astronomical physics --- Astronomy --- Cosmic physics --- Geography --- Science and space --- Space research --- Cosmology --- Science --- Geological physics --- Terrestrial physics --- Earth sciences

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When the stream of plasma emitted from the Sun (the solar wind) encounters Earth's magnetic field, it slows down and flows around it, leaving behind a cavity, the magnetosphere. The magnetopause is the surface that separates the solar wind on the outside from the Earth's magnetic field on the inside. Because the solar wind moves at supersonic speed, a bow shock must form ahead of the magnetopause that acts to slow the solar wind to subsonic speeds. Magnetopause, bow shock and their environs are rich in exciting processes in collisionless plasmas, such as shock formation, magnetic reconnection, particle acceleration and wave-particle interactions. They are interesting in their own right, as part of Earth's environment, but also because they are prototypes of similar structures and phenomena that are ubiquitous in the universe, having the unique advantage that they are accessible to in situ measurements. The boundaries of the magnetosphere have been the target of direct in-situ measurements since the beginning of the space age. But because they are constantly moving, changing their orientation, and undergoing evolution, the interpretation of single-spacecraft measurements has been plagued by the fundamental inability of a single observer to unambiguously distinguish spatial from temporal changes. The boundaries are thus a prime target for the study by a closely spaced fleet of spacecraft. Thus the Cluster mission, with its four spacecraft in a three-dimensional configuration at variable separation distances, represents a giant step forward. The present 20th volume of the ISSI Space Science Series represents the first synthesis of the exciting new results obtained in the first few years of the Cluster mission.

Magnetosphere. --- Magnetopause. --- Solar wind. --- Magnetosphere --- Atmosphere, Upper --- Plasma, Solar --- Solar plasma --- Wind, Solar --- Solar activity --- Stellar winds --- Heliosphere (Astrophysics) --- Upper atmosphere --- Planetology. --- Physical geography. --- Astronomy. --- Classical Electrodynamics. --- Astrophysics and Astroparticles. --- Geophysics/Geodesy. --- Astronomy, Astrophysics and Cosmology. --- Astronomy, Observations and Techniques. --- Geography --- Planetary sciences --- Planetology --- Optics. --- Electrodynamics. --- Astrophysics. --- Geophysics. --- Observations, Astronomical. --- Astronomy—Observations. --- Astronomical physics --- Astronomy --- Cosmic physics --- Physics --- Geological physics --- Terrestrial physics --- Earth sciences --- Astronomical observations --- Observations, Astronomical --- Light --- Dynamics --- Observations.

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The essential introduction to magnetic reconnection—written by a leading pioneer of the fieldPlasmas comprise more than 99 percent of the visible universe; and, wherever plasmas are, magnetic reconnection occurs. In this common and yet incompletely understood physical process, oppositely directed magnetic fields in a plasma meet, break, and then reconnect, converting the huge amounts of energy stored in magnetic fields into kinetic and thermal energy. In Magnetic Reconnection, Masaaki Yamada offers an illuminating synthesis of modern research and advances on this important topic. Magnetic reconnection produces such phenomena as solar flares and the northern lights, and occurs in nuclear fusion devices. A better understanding of this crucial cosmic activity is essential to comprehending the universe and varied technological applications, such as satellite communications. Most of our knowledge of magnetic reconnection comes from theoretical and computational models and laboratory experiments, but space missions launched in recent years have added up-close observation and measurements to researchers’ tools. Describing the fundamental physics of magnetic reconnection, Yamada connects the theory with the latest results from laboratory experiments and space-based observations, including the Magnetic Reconnection Experiment (MRX) and the Magnetospheric Multiscale (MMS) Mission. He concludes by considering outstanding problems and laying out a road map for future research.Aimed at advanced graduate students and researchers in plasma astrophysics, solar physics, and space physics, Magnetic Reconnection provides cutting-edge information vital area of scientific investigation.

Magnetic reconnection. --- SCIENCE / Physics / Magnetism. --- Acceleration. --- Accretion disk. --- Ampere. --- Annihilation. --- Astrophysical plasma. --- Astrophysics. --- Bremsstrahlung. --- Collision frequency. --- Collisionality. --- Coronal loop. --- Coronal mass ejection. --- Coulomb collision. --- Current density. --- Current sheet. --- Cyclotron. --- Debye length. --- Diffusion layer. --- Dissipation. --- Drift velocity. --- Dynamo theory. --- Electric field. --- Electrical resistivity and conductivity. --- Electron temperature. --- Electrostatics. --- Energy transformation. --- Experimental physics. --- Fermi acceleration. --- Feynman diagram. --- Field effect (semiconductor). --- Field line. --- Fine structure. --- Flux tube. --- Fusion power. --- Gauge theory. --- Gyroradius. --- Hall effect. --- Inductance. --- Induction equation. --- Instability. --- Interferometry. --- Ion acoustic wave. --- Ionization. --- Kinetic theory of gases. --- Kink instability. --- Landau damping. --- Langmuir probe. --- Length scale. --- Lorentz force. --- Madison Symmetric Torus. --- Magnetar. --- Magnetic confinement fusion. --- Magnetic diffusivity. --- Magnetic dipole. --- Magnetic energy. --- Magnetic field. --- Magnetic flux. --- Magnetic helicity. --- Magnetization. --- Magnetohydrodynamics. --- Magnetopause. --- Magnetosheath. --- Magnetosonic wave. --- Magnetosphere. --- Maxwell–Boltzmann distribution. --- Mean free path. --- Momentum transfer. --- Neutral beam injection. --- Nonlinear optics. --- Nuclear fusion. --- Paramagnetism. --- Particle physics. --- Pitch angle (particle motion). --- Plasma (physics). --- Plasma acceleration. --- Plasma oscillation. --- Plasma parameter. --- Plasma parameters. --- Plasma stability. --- Plasmoid. --- Quadrupole. --- Relativistic plasma. --- Reversed field pinch. --- Safety factor (plasma physics). --- Scattering. --- Skin effect. --- Solar flare. --- Spacecraft. --- Spatial scale. --- Spheromak. --- Stark effect. --- Substorm. --- Synchrotron radiation. --- Thermodynamic equilibrium. --- Thomson scattering. --- Tokamak. --- Two-dimensional space. --- Van Allen radiation belt. --- Weibel instability. --- X-ray. --- Annihilation, Magnetic field --- Magnetic field annihilation --- Magnetic field line merging --- Merging, Magnetic field line --- Reconnection, Magnetic --- Reconnection (Astronomy) --- Astrophysics --- Geophysics --- Magnetic fields