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Автор Coroniti, F. V.
Автор Scarf, F. L.
Автор Kennel, C. F.
Автор Tsurutani, B. T.
Автор Smith, E. J.
Дата выпуска 1988
dc.description The slow shocks which have been observed in the distant geomagnetic tail by ISEE 3 do not exhibit the large‐amplitude magnetic field rotations which are theoretically expected. A possible explanation is that the rotational trailing wave train is resistively damped by strong lower hybrid drift turbulence excited in the shock front. Magnetic wave spectra for three slow shocks are constructed from the ISEE 3 dc magnetometer and search coil experiments. The observed magnetic amplitudes near the lower hybrid frequency are below the level at which anomalous resistance would damp the slow shock magnetic rotations.
Формат application.pdf
Копирайт Copyright 1988 by the American Geophysical Union.
Тема IONOSPHERE
Тема Plasma waves and instabilities
Тема MAGNETOSPHERIC PHYSICS
Тема Magnetotail
Тема Plasma waves and instabilities
Тема NONLINEAR GEOPHYSICS
Тема Nonlinear waves, shock waves, solitons
Тема Turbulence
Тема SPACE PLASMA PHYSICS
Тема Shock waves
Тема Turbulence
Название A search for lower hybrid drift turbulence in slow shocks
Тип article
DOI 10.1029/JA093iA04p02553
Electronic ISSN 2156-2202
Print ISSN 0148-0227
Журнал Journal of Geophysical Research: Space Physics
Том 93
Первая страница 2553
Последняя страница 2561
Выпуск A4
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