Plasma waves in planetary magnetospheres

Publisher Website
Google Scholar
Abstract
The studies of magnetospheric plasma waves in the 1979–1982 quadrennium have included not only intensive studies of plasma waves in the Earth's magnetosphere but also, for the first time, in situ observations and detailed analyses of plasma waves in the magnetospheres of Jupiter and Saturn. While much of the research has involved the continuing identification and classification of plasma wave phenomena in the magnetospheres, increasingly greater emphasis has been placed on understanding the sources of the plasma waves and the interactions of plasma waves with the particles. Many studies have also shown that plasma wave measurements may be used to discern numerous geophysical boundaries and parameters.At the earth, significant progress in plasma wave research has been made that has increased our understanding of wave‐particle interactions and their effects, throughout the magnetosphere from the auroral ionosphere out to the bow shock and back into the tail. Observations of auroral kilometric radiation both in the source region and far from it have provided much new information about this intense emission. Details of the fine structure of the radiation and its polarization and propagation characteristics along with particle distribution and other plasma wave measurements in the source region have provided valuable inputs to various generation theories. Similar progress has also been made in understanding electron cyclotron harmonic emissions and nonthermal continuum radiation. Detailed characterizations of plasma wave phenomena reported during this quadrennium in the plasmasphere, outer magnetosphere, magnetopause, magnetosheath and tail regions have been important in assessing the impact of the waves on the particle distributions and vise versa.