Observational Evidence of Dissipative Small Scale Processes: Geotail Spacecraft Observation and Simulation of Electrostatic Solitary Waves |
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Authors: | Y Omura H Kojima T Umeda H Matsumoto |
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Institution: | (1) Radio Science Center for Space and Atmosphere, Kyoto University, Japan |
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Abstract: | In recent spacecraft observations, coherent microscale structures such as electrostatic solitary waves are observed in various
regions of the magnetosphere. The Geotail spacecraft observation has shown that these solitary waves are associated with high
energy non-thermal electrons flowing along the magnetic field. The solitary structures are generated as a result of a long
time evolution of coherent nonlinear trapping of electrons as found in bump-on-tail, bi-stream and Buneman instabilities.
It is noted that these solitary waves can be generated at distant regions far away from the spacecraft locations, because
these trapped electrons, or electron holes, are drifting much faster than the local thermal plasmas. Some of the solitary
waves are accompanied by perpendicular electric fields indicating that two-or three-dimensional potential structures are passing
by the spacecraft. Depending on the local plasma parameters, these multi-dimensional solitary structures couple with perpendicular
modes such as electrostatic whistler modes and lower-hybrid modes. In a long time evolution, these perpendicular modes are
dissipated via self-organization of small solitary potentials, leading to formation of one-dimensional potential troughs as
observed in the deep magnetotail. The above dissipative small-scale processes are reproduced in particle simulations, and
they can be used for diagnostics of electron dynamics from spacecraft observation of multi-dimensional solitary waves in various
regions of the magnetosphere.
This revised version was published online in July 2006 with corrections to the Cover Date. |
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