An observed characteristic of concurrent magnetic field and electron precipitation pulsations

Details An observed characteristic of concurrent magnetic field and electron precipitation pulsations An observed characteristic of concurrent magnetic field and electron precipitation pulsations

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981jatp...43..675h&link_type=abstract

Journal of Atmospheric and Terrestrial Physics, vol. 43, July 1981, p. 675-678.

Physics

4

Electron Precipitation, Geomagnetic Pulsations, Ionospheric Conductivity, Magnetically Trapped Particles, Magnetohydrodynamic Waves, Plasma-Particle Interactions, Power Spectra, Riometers, Space Plasmas

Scientific paper

In each case for a collection of seven large-amplitude events, spectral peaks in the 1 to 10 mHz range for electron precipitation pulsations were observed to correspond to spectral peaks for concurrent magnetic field pulsations. The converse is not true, i.e. a magnetic field pulsation spectral peak need not correspond to a precipitation spectral peak, and in fact there may not even be a concurrent precipitation pulsation event. The data are consistent with occurrences of interactions between a portion of the hydromagnetic wave spectrum and trapped electrons in the equatorial region of the field line of the site.

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