Response of energetic particles to magnetospheric ultra-low-frequency waves

Details Response of energetic particles to magnetospheric ultra-low-frequency waves Response of energetic particles to magnetospheric ultra-low-frequency waves

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jhatd..11..255t&link_type=abstract

Johns Hopkins APL Technical Digest (ISSN 0270-5214), vol. 11, July-Dec. 1990, p. 255-263. Research supported by NASA.

Physics

Space Physics

Ampte (Satellites), Earth Magnetosphere, Energetic Particles, Magnetohydrodynamic Waves, Magnetospheric Instability, Wave Propagation, Kinetics, Magnetic Fields, Magnetotails, Plasma Waves, Power Spectra, Standing Waves

Scientific paper

ULF waves in the space physics context are the lowest-frequency plasma waves propagating in the earth's magnetosphere. Although the propagation of the waves is explained in MHD theory, excitation of the waves involves not only MHD but also kinetic processes. This article describes how in situ magnetic field and particle measurements can be used to distinguish the basic properties of ULF waves, including the azimuthal wave number of the standing wave structure and the propagation direction. Examples are taken from observations with the AMPTE/CCE spacecraft.

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