Azimuthal phase speeds of field line resonances driven by Kelvin-Helmholtz unstable waveguide modes

Author:

Mills Katharine J.,Wright Andrew N.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference25 articles.

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2. Three-dimensional plasma observations near the outer magnetospheric boundary;Eastman;J. Geophys. Res.,1985

3. The dependence of 1Yigh-latitude Pc5 wave power on solar wind velocity and on the phase of high-speed solar wind streams;Engebretson;J. Geophys. Res.,1998

4. ULF high- and low-m field line resonances observed with the Super Dual Auroral Radar Network;Fenrich;J. Geophys. Res.,1995

5. MHD waves generated by the Kelvin-Helmholtz instability in a nonuniform magnetosphere;Fujita;J. Geophys. Res.,1996

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