Physics
Scientific paper
Jun 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jgr....98.9189o&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 98, no. A6, p. 9189-9199.
Physics
1
Geomagnetic Tail, Magnetic Field Reconnection, Magnetic Signatures, Plasma Waves, Ray Tracing, Data Simulation, Signature Analysis
Scientific paper
An MHD simulation was performed to obtain a self-consistent model of magnetic field and plasma density near the X point reconnection region. The MHD model was used to perform extensive ray tracing calculations in order to clarify the propagation characteristics of the plasma waves near the X point reconnection region. The dynamic wave spectra possibly observed by the Geotail spacecraft during a typical cross-tail trajectory are reconstructed. By comparing the extensive ray tracing calculations with the plasma wave data from Geotail, it is possible to perform a kind of 'remote sensing' to identify the location and structure of potential X point reconnection regions.
Green James L.
Omura Yoshiharu
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