Physics of Collisionless Shocks Space Plasma Shock Waves ISSI Scientific Report Series Book 12 2013 André Balogh Rudolf A Treumann lesen HKF

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PDF Reader Physics of Collisionless Shocks Space Plasma Shock Waves ISSI Scientific Report Series Book 12 2013 André Balogh Rudolf A Treumann BQS

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The present book provides a contemporary systematic treatment of shock waves in high-temperature collisionless plasmas as are encountered in near Earth space and in Astrophysics. It consists of two parts. Part I develops the complete theory of shocks in dilute hot plasmas under the assumption of absence of collisions among the charged particles  when the interaction is mediated solely by the self-consistent electromagnetic fields. Such shocks are naturally magnetised implying that the magnetic field plays an important role in their evolution and dynamics. This part treats subcritical shocks which dissipate flow energy by generating anomalous resistance or viscosity. The main emphasis is, however, on super-critical shocks where the anomalous dissipation is insufficient to retard the upstream flow. These shocks, depending on the direction of the upstream magnetic field, are distinguished as quasi-perpendicular and quasi-parallel shocks which exhibit different behaviours, reflecting particles back upstream and generating high electromagnetic wave intensities. Particle acceleration and turbulence at such shocks become possible and important. Part II treats planetary bow shocks and the famous Heliospheric Termination shock as examples of two applications of the theory developed in part I.
ebook,André Balogh, Rudolf A. Treumann,Physics of Collisionless Shocks Space Plasma Shock Waves (ISSI Scientific Report Series Book 12),Springer,Astronautics,Astrophysics,Astrophysics and Astroparticles,B,Bow Shocks; Collisionless Shocks; Internal and External Shocks; Interstellar Matter; Particle Acceleration; Solar Corona; Stellar Winds; Supercritical Flows; Supercritical Shocks; Termination Shocks,Bow Shocks;Collisionless Shocks;Internal and External Shocks;Interstellar Matter;Particle Acceleration;Solar Corona;Stellar Winds;Supercritical Flows;Supercritical Shocks;Termination Shocks,Collisionless plasmas,Monograph Series, any,NUCLEAR PHYSICS,Non-Fiction,Physics,Physics - Astrophysics,Physics - Nuclear,Physics and Astronomy,Physik, Astronomie / Astronomie,Plasma (Ionized gases),Plasma astrophysics,Plasma physics,SCI/TECH,SCIENCE / Physics / Astrophysics,SCIENCE / Physics / Nuclear,Scholarly/Undergraduate,Science,Science/Math,Science/Mathematics,Science/Physics - Nuclear,Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics),Space sciences,United States,Physics - Astrophysics,Physics - Nuclear,SCIENCE / Physics / Astrophysics,SCIENCE / Physics / Nuclear,Science/Physics - Nuclear,Science,Nuclear Physics,Science/Mathematics,Astronautics,Physik, Astronomie / Astronomie

Physics of Collisionless Shocks Space Plasma Shock Waves ISSI Scientific Report Series Book 12 2013 André Balogh Rudolf A Treumann Reviews :

The present book provides a contemporary systematic treatment of shock waves in high-temperature collisionless plasmas as are encountered in near Earth space and in Astrophysics. It consists of two parts. Part I develops the complete theory of shocks in dilute hot plasmas under the assumption of absence of collisions among the charged particles  when the interaction is mediated solely by the self-consistent electromagnetic fields. Such shocks are naturally magnetised implying that the magnetic field plays an important role in their evolution and dynamics. This part treats subcritical shocks which dissipate flow energy by generating anomalous resistance or viscosity. The main emphasis is, however, on super-critical shocks where the anomalous dissipation is insufficient to retard the upstream flow. These shocks, depending on the direction of the upstream magnetic field, are distinguished as quasi-perpendicular and quasi-parallel shocks which exhibit different behaviours, reflecting particles back upstream and generating high electromagnetic wave intensities. Particle acceleration and turbulence at such shocks become possible and important. Part II treats planetary bow shocks and the famous Heliospheric Termination shock as examples of two applications of the theory developed in part I.

ebook,André Balogh, Rudolf A. Treumann,Physics of Collisionless Shocks Space Plasma Shock Waves (ISSI Scientific Report Series Book 12),Springer,Astronautics,Astrophysics,Astrophysics and Astroparticles,B,Bow Shocks; Collisionless Shocks; Internal and External Shocks; Interstellar Matter; Particle Acceleration; Solar Corona; Stellar Winds; Supercritical Flows; Supercritical Shocks; Termination Shocks,Bow Shocks;Collisionless Shocks;Internal and External Shocks;Interstellar Matter;Particle Acceleration;Solar Corona;Stellar Winds;Supercritical Flows;Supercritical Shocks;Termination Shocks,Collisionless plasmas,Monograph Series, any,NUCLEAR PHYSICS,Non-Fiction,Physics,Physics - Astrophysics,Physics - Nuclear,Physics and Astronomy,Physik, Astronomie / Astronomie,Plasma (Ionized gases),Plasma astrophysics,Plasma physics,SCI/TECH,SCIENCE / Physics / Astrophysics,SCIENCE / Physics / Nuclear,Scholarly/Undergraduate,Science,Science/Math,Science/Mathematics,Science/Physics - Nuclear,Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics),Space sciences,United States,Physics - Astrophysics,Physics - Nuclear,SCIENCE / Physics / Astrophysics,SCIENCE / Physics / Nuclear,Science/Physics - Nuclear,Science,Nuclear Physics,Science/Mathematics,Astronautics,Physik, Astronomie / Astronomie

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Product details File Size 21239 KB Print Length 500 pages Publisher Springer; 2013 edition (January 4, 2013) Publication Date January 4, 2013 Sold by  Services LLC Language English ASIN B00BLQ03QI

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