Physics of Collisionless Shocks: Space Plasma Shock Waves
Gespeichert in:
| Hauptverfasser: | , |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
New York, NY [u.a.]
Springer
2013
|
| Schriftenreihe: | ISSI Scientific Report Series
12 |
| Schlagworte: | |
| Online-Zugang: | TUM01 UBT01 Volltext Inhaltsverzeichnis Abstract |
| Beschreibung: | 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 both subcritical shocks, which dissipate flow energy by generating anomalous resistance or viscosity, and supercritical shocks. 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. |
| Beschreibung: | 1 Online-Ressource |
| ISBN: | 9781461460992 |
| DOI: | 10.1007/978-1-4614-6099-2 |
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| 500 | |a 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 both subcritical shocks, which dissipate flow energy by generating anomalous resistance or viscosity, and supercritical shocks. 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. | ||
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Datensatz im Suchindex
| _version_ | 1804150074444349440 |
|---|---|
| adam_text | PHYSICS OF COLLISIONLESS SHOCKS
/ BALOGH, ANDRE
: 2013
TABLE OF CONTENTS / INHALTSVERZEICHNIS
PART I
THE SHOCK PROBLEM
EQUATIONS AND MODELS
SUBCRITICAL SHOCKS
QUASI-PERPENDICULAR SUPERCRITICAL SHOCKS
QUASI-PARALLEL SUPERCRITICAL SHOCKS
PARTICLE ACCELERATION
FINAL REMARKS
PART II
INTRODUCTION.-PLANETARY BOW SHOCKS.-THE HELIOSPHERIC TERMINATION
SHOCK
DIESES SCHRIFTSTUECK WURDE MASCHINELL ERZEUGT.
PHYSICS OF COLLISIONLESS SHOCKS
/ BALOGH, ANDRE
: 2013
ABSTRACT / INHALTSTEXT
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 BOTH SUBCRITICAL SHOCKS, WHICH DISSIPATE FLOW ENERGY BY
GENERATING ANOMALOUS RESISTANCE OR VISCOSITY,AND SUPERCRITICAL SHOCKS.
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.
DIESES SCHRIFTSTUECK WURDE MASCHINELL ERZEUGT.
|
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| author | Balogh, André Treumann, Rudolf A. 1942- |
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| isbn | 9781461460992 |
| language | English |
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| spelling | Balogh, André Verfasser aut Physics of Collisionless Shocks Space Plasma Shock Waves André Balogh ; Rudolf A. Treumann New York, NY [u.a.] Springer 2013 1 Online-Ressource txt rdacontent c rdamedia cr rdacarrier ISSI Scientific Report Series 12 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 both subcritical shocks, which dissipate flow energy by generating anomalous resistance or viscosity, and supercritical shocks. 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. Physics Astrophysics Extraterrestrial Physics, Space Sciences Astrophysics and Astroparticles Plasma Physics Treumann, Rudolf A. 1942- Verfasser (DE-588)115464611 aut Erscheint auch als Druckausgabe 978-1-4614-6098-5 ISSI Scientific Report Series 12 (DE-604)BV040611034 12 https://doi.org/10.1007/978-1-4614-6099-2 Verlag Volltext Springer Fremddatenuebernahme application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=025730933&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis Springer Fremddatenuebernahme application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=025730933&sequence=000003&line_number=0002&func_code=DB_RECORDS&service_type=MEDIA Abstract |
| spellingShingle | Balogh, André Treumann, Rudolf A. 1942- Physics of Collisionless Shocks Space Plasma Shock Waves ISSI Scientific Report Series Physics Astrophysics Extraterrestrial Physics, Space Sciences Astrophysics and Astroparticles Plasma Physics |
| title | Physics of Collisionless Shocks Space Plasma Shock Waves |
| title_auth | Physics of Collisionless Shocks Space Plasma Shock Waves |
| title_exact_search | Physics of Collisionless Shocks Space Plasma Shock Waves |
| title_full | Physics of Collisionless Shocks Space Plasma Shock Waves André Balogh ; Rudolf A. Treumann |
| title_fullStr | Physics of Collisionless Shocks Space Plasma Shock Waves André Balogh ; Rudolf A. Treumann |
| title_full_unstemmed | Physics of Collisionless Shocks Space Plasma Shock Waves André Balogh ; Rudolf A. Treumann |
| title_short | Physics of Collisionless Shocks |
| title_sort | physics of collisionless shocks space plasma shock waves |
| title_sub | Space Plasma Shock Waves |
| topic | Physics Astrophysics Extraterrestrial Physics, Space Sciences Astrophysics and Astroparticles Plasma Physics |
| topic_facet | Physics Astrophysics Extraterrestrial Physics, Space Sciences Astrophysics and Astroparticles Plasma Physics |
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