Physics
Scientific paper
Apr 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998jgr...103.6621l&link_type=abstract
Journal of Geophysical Research, Volume 103, Issue A4, p. 6621-6632
Physics
10
Interplanetary Physics: Plasma Waves And Turbulence
Scientific paper
A new approach is proposed to identify mirror waves based on the 90° phase difference between the magnetic field and plasma fluctuations. Magnetosheath observations, the linear MHD theory, and one-dimensional hybrid simulations support that the 90° phase difference is a special character for mirror waves. This phase difference is independent of Doppler shift which means that our result remains the same in both the satellite (laboratory) and the plasma frames of reference. Therefore it is useful to distinguish mirror waves from slow waves which also have an anticorrelation (i.e., 180° out of phase) relationship between magnetic field strength and plasma density fluctuations. The time evolution in the later stage shows that the dominant perturbed components are the magnetic field fluctuation along the background magnetic field
Chao Jerry K.
Lee Clarence L.
Li Yadong
Lin Cheng-Horng
Song Paul
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