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Physics of Collisionless Shocks - Space Plasma Shock Waves (Paperback, 2013 ed.)
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Physics of Collisionless Shocks - Space Plasma Shock Waves (Paperback, 2013 ed.)
Series: ISSI Scientific Report Series, 12
Expected to ship within 10 - 15 working days
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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.
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