£111.93

Springer Plasma Astrophysics, Part II: Reconnection and Flares

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Description

Explore the complex world of magnetic fields and plasma phenomena with Plasma Astrophysics, Part II: Reconnection and Flares. Published by Springer as part of the Astrophysics and Space Science Library, this volume provides a deep look into how magnetic fields are generated in astrophysical plasma due to high conductivity. From the large-scale magnetic fields found in spiral galaxies like M51 to the extreme magnetic strengths of magnetars, this text covers a wide range of cosmic scales. Learn about the potential origins of these fields, including the amplification of seed fields through turbulent galactic dynamos. This book is an essential resource for those studying how magnetic fields correlate with optical spiral arms and the fundamental physics governing the strongest magnets in space. Whether you are researching galactic structures or high-energy astrophysical events, this volume offers detailed insights into the mechanics of reconnection and flares.

Key Features

Part of the professional Astrophysics and Space Science Library (Volume 341) for academic research.

Covers the generation of magnetic fields in astrophysical plasma driven by high conductivity.

Analyzes magnetic field correlations in spiral galaxies such as M51.

Explores the role of turbulent galactic dynamos in amplifying small seed fields.

Provides information on the strongest magnets in space, including magnetars.

Examines magnetic field strengths ranging from kiloparsec scales to extreme cosmic environments.

Product Specifications

Format
paperback
Domain
Amazon UK
Release Date
16 December 2010
Listed Since
06 July 2010

Barcode

No barcode data available

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