Spatiotemporal Variability and Propagation of Equatorial Noise Observed by Cluster

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Transit time scattering of energetic electrons due to equatorially confined magnetosonic waves (2010, background): “, 1994], and some radial translation which can lead to a nonlocal fci spacing between the MS harmonic lines [Santolík et al., 2002].”
Systematic analysis of equatorial noise below the lower hybrid frequency (2004, background): “(12) of Santolı́k et al. (2003). It is defined as F=1− √ w3/ √ w1, where w1 and w3 are, respectively, the maximum and the minimum singular values of the magnetic spectral matrix.”
Global simulation of magnetosonic wave instability in the storm time magnetosphere (2010, background): “magnetic equator [Russell et al., 1970; Santolík et al., 2002; Němec et al., 2005] both inside and outside the plasmapause.”
Global distribution of equatorial magnetosonic waves observed by THEMIS (2013, methodology): “, 1982] and Cluster spacecraft [Santolik et al., 2002] provided evidence that the locally generated wave spectra match the harmonics of the local proton gyrofrequency, even though the waves can propagate with a significant radial component.”