Magnetic pumping of whistler waves by tether current modulation

Magnetic excitation of whistlers by a square array of electrodynamic tethers is discussed. The array is made of perpendicular rows of tethers that carry equal, uniform, and time‐modulated currents at equal frequency with a 90° phase shift. The array would fly vertical in the orbital equatorial plane...

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Bibliographic Details
Published inJournal of Geophysical Research. B. Solid Earth Vol. 115; no. A2
Main Authors Sanchez-Arriaga, G., Sanmartin, J. R.
Format Journal Article
LanguageEnglish
Published Washington, DC Blackwell Publishing Ltd 13.02.2010
American Geophysical Union
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Summary:Magnetic excitation of whistlers by a square array of electrodynamic tethers is discussed. The array is made of perpendicular rows of tethers that carry equal, uniform, and time‐modulated currents at equal frequency with a 90° phase shift. The array would fly vertical in the orbital equatorial plane, which is perpendicular to the geomagnetic field B0 when its tilt is ignored. The array radiates a whistler wave along B0. A parametric instability due to pumping by the background magnetic field through the radiated wave gives rise to two unstable coupled whistler perturbations. The growth rate is maximum for perturbations with wave vector at angles 38.36° and 75.93° from B0. For an experiment involving a wavefront that moves with the orbiting array, which might serve to study nonlinear wave interactions and turbulence in space plasmas, characteristic values of growth rate and parameters, such as the number of tethers and their dimensions and distances in the array, are discussed for low Earth orbit ambient conditions.
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ISSN:0148-0227
2169-9380
2156-2202
2169-9402
DOI:10.1029/2009JA014478