Introduction to Space PhysicsMargaret G. Kivelson, Christopher T. Russell Cambridge University Press, 1995 M04 28 - 568 pages All aspects of space plasmas in the Solar System are introduced and explored in this text for senior undergraduate and graduate students. Introduction to Space Physics provides a broad, yet selective, treatment of the complex interactions of the ionized gases of the solar terrestrial environment. The book includes extensive discussion of the Sun and solar wind, the magnetized and unmagnetized planets, and the fundamental processes of space plasmas including shocks, plasma waves, ULF waves, wave particle interactions, and auroral processes. The text devotes particular attention to space plasma observations and integrates these with phenomenological and theoretical interpretations. Highly coordinated chapters, written by experts in their fields, combine to provide a comprehensive introduction to space physics. Based on an advanced undergraduate and graduate course presented in the Department of Earth and Space Sciences at the University of California, Los Angeles, the text will be valuable to both students and professionals in the field. |
Contents
A BRIEF HISTORY OF SOLARTERRESTRIAL PHYSICS | 1 |
PHYSICS OF SPACE PLASMAS | 27 |
THE SUN AND ITS MAGNETOHYDRODYNAMICS | 58 |
Problems | 89 |
Solar Corona | 96 |
Solar Wind | 124 |
Additional Reading | 163 |
IONOSPHERES | 183 |
PULSATIONS AND MAGNETOHYDRODYNAMIC | 330 |
PLASMA WAVES | 356 |
MAGNETOSPHERIC DYNAMICS | 400 |
Standard Indices of Geomagnetic | 451 |
Additional Reading | 457 |
Additional Reading | 500 |
Notation Vector Identities and Differential | 521 |
Fundamental Constants and Plasma | 529 |
PLASMA INTERACTIONS WITH UNMAGNETIZED | 203 |
THE MAGNETOPAUSE MAGNETOTAIL | 227 |
MAGNETOSPHERIC CONFIGURATION | 288 |
| 545 | |
| 563 | |
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Common terms and phrases
accelerated Alfvén speed Alfvén wave altitude Ampère's law angle atmosphere auroral average axis boundary layer bow shock Chapter charged particles collisions component constant convection coordinate system corona current sheet dayside density diffusion dipole field direction discussed dispersion relation distance distribution drift earth electric field electrons emissions energy equation equatorial plane field strength field-aligned fluid flux tube foreshock frequency geomagnetic gradient gyroradius heating illustrated in Figure increases instability interaction interplanetary ionization ionosphere ions latitude Mach number magnetic field magnetic reconnection magnetic-field lines magnetopause magnetosheath magnetosphere magnetotail mass measured momentum motion move neutral nightside normal observed occur orbit parallel parameters perpendicular perturbations phase planetary plasma flow plasma sheet plasmasphere polar cap propagation protons radius reconnection region ring current rotation shown in Figure shows solar wind solution space spacecraft speed substorm surface tail lobes temperature thermal tion upstream variations vector velocity x-line

