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Whistler wave dispersion measurements near the ion gyro frequency

MPS-Authors
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Stark,  A.
VINETA, Max Planck Institute for Plasma Physics, Max Planck Society;
Stellarator Scenario Development (E5), Max Planck Institute for Plasma Physics, Max Planck Society;

Franck,  C.
Max Planck Society;

/persons/resource/persons109244

Grulke,  O.
VINETA, Max Planck Institute for Plasma Physics, Max Planck Society;
Stellarator Scenario Development (E5), Max Planck Institute for Plasma Physics, Max Planck Society;

/persons/resource/persons109625

Klinger,  T.
Stellarator Scenario Development (E5), Max Planck Institute for Plasma Physics, Max Planck Society;
VINETA, Max Planck Institute for Plasma Physics, Max Planck Society;

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Citation

Stark, A., Franck, C., Grulke, O., & Klinger, T. (2003). Whistler wave dispersion measurements near the ion gyro frequency. In J. Meichsner, D. Loffhagen, & H.-E. Wagner (Eds.), 26th International Conference on Phenomena in Ionized Gases. Vol. 4 (pp. 163-164).


Cite as: http://hdl.handle.net/11858/00-001M-0000-0027-3C3F-5
Abstract
Investigation of ion whistler waves under laboratory conditions is difficult because of the long wavelength. In the VINETA device electromagnetic waves around the ion gyro frequency have been successfully launched. For frequencies above the ion gyro frequency the waves are identified as R-waves. Below the ion gyro frequency the measurements cannot be explained by R-wave or L-wave dispersion alone. In a heuristic way the observed dispersion is described by the difference wavelength of R-wave and L-wave.