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Magnetic Helicity, Spheromaks, Solar Corona Loops, And Astrophysical Jets

relaxation, is a fundamental concept that unifies understanding of spheromaks, solar corona loops, interplanetary magnetic clouds, and astrophysical;

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Advances in Plasma Astrophysics (IAU S274)

different fields examine topics including: the origin and dynamics of magnetic fields in astrophysical systems (the dynamo problem); the origin of x;

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Astrophysical Jets and Beams

role they play in many long-standing problems in astrophysics. It covers the major discoveries in gamma-ray bursts, solar and stellar jets and;

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Solar Flare Loops Observations and Interpretations

This book provides results of analysis of typical solar events, statistical analysis, the diagnostics of energetic electrons and magnetic;

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Fundamentals of Plasma Physics

. Magnetohydrodynamic equilibrium and stability are tackled with emphasis on the topological concepts of magnetic helicity and self-organization. Advanced;

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Solar And Astrophysical Dynamos And Magnetic Activity (Iau S

advanced students and researchers, as a summary of hot topics related to the solar and astrophysical dynamos and magnetic activity.;

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Cambridge Astrophysics

corona. Plasma loops cover a wide range of sizes, and range in temperature from tens of thousands to millions of degrees. They not only define;

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Cambridge Astrophysics

corona. Plasma loops cover a wide range of sizes, and range in temperature from tens of thousands to millions of degrees. They not only define;

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Collisionless Shocks in Space Plasmas

Shock waves are an important feature of solar system plasmas, from the solar corona out to the edge of the heliosphere. This engaging;

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Solar Surface Magnetism

While the emergence and evolution of solar surface magnetic flux reveals what goes on in the solar interior, the interplay of convection;

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Magnetic Reconnection in Plasmas

astrophysical phenomena and dynamo theory, with emphasis on the solar and geodynamo, as well as magnetospheric substorms, the most spectacular;

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Magnetohydrodynamics and Fluid Dynamics

helicity reconnection hypothesis for magnetic fields in highly conducting plasmas, and the magnetic helicity of Alfven simple waves, MHD;

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Magnetohydrodynamics Handbook

tokamaks, magnetic relaxation procedure in spheromaks, and the creation and stability of field-reversed configuration have been provided in this;

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Physics of Plasmas

research using magnetic confinement of Deuterium plasma, solar physics with its plasma loops reaching high into the corona, sunspots and solar wind;

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Cambridge Monographs on Plasma Physics

astrophysical phenomena and dynamo theory, with emphasis on the solar and geodynamo, as well as magnetospheric substorms, the most spectacular;

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Space Physics and Aeronomy Volume 1 - At the Doors tep of Our Star - Solar Physics and Solar Wind

magnetic field and its radiative output Description of solar atmospheric phenomena such as spicules and jets New developments in understanding;

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Magneto-Fluid Dynamics

This book provides an understanding of the physics at work in sunspots and solar coronal loops, and offers a new approach to Magneto-Fluid;

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Jets in Young Stellar Objects

This volume presents the results of the workshop discussions on the jet phenomenon on different astrophysical scales and covers;

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Self-Exciting Fluid Dynamos

Exploring the origins and evolution of magnetic fields in planets, stars and galaxies, this book gives a basic introduction to;

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Self-Exciting Fluid Dynamos

Exploring the origins and evolution of magnetic fields in planets, stars and galaxies, this book gives a basic introduction to;

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The Magnetic Universe

Magnetic fields permeate our vast universe, urging electrically charged particles on their courses, powering solar and stellar flares, and;

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Physics of Solar and Stellar Coronae

-main sequence stars. Detailed models for the hot plasmas typically contained in magnetic loops in both stellar and solar coronae are presented;

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Magnetic Reconnection

Magnetic reconnection is at the core of many dynamic phenomena in the universe, such as solar flares, geomagnetic substorms and tokamak;

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Mass Supply and Flows in the Solar Corona

and flows in the solar corona, focusing on: fine scale structures; loops and prominences; streamers; and coronal holes and solar wind. Each;

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Microphysics of Cosmic Plasmas

and solar system plasmas as a phenomenological description of their dynamic properties on all scales; observational, theoretical and modelling;

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Coronal Seismology: Waves and Oscillations in Stellar Coronae

astrophysics, magneto-hydrodynamics and coronal magnetic structures, taking into account the full range of available observation techniques -- from;

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UV and X-Ray Spectroscopy of Laboratory and Astrophysical Plasmas

superb data on the solar corona. In the laboratory, the development of ion-trap facilities and novel laser experiments are providing vital new;

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