ULF waves in the solar wind as direct drivers of magnetospheric pulsations

297 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

The Upgraded CARISMA Magnetometer Array in the THEMIS Era (2008, background): “…Kelvin-Helmholtz instability (e.g. McKenzie 1970; Pu and Kivelson 1983; Miura 1992; Mann et al. 1999; Fairfield et al. 2007, and references therein); • Solar wind dynamic pressure fluctuations (e.g. Kepko et al., 2002; Mathie and Mann 2000c); and many others (see also Angelopoulos 2008).”
Evolution and characteristics of global Pc5 ULF waves during a high solar wind speed interval (2005, methodology): “…Kelvin-Helmholtz Instability (KHI) via surface waves [e.g., Southwood, 1974; Chen and Hasegawa, 1974], direct solar wind ram pressure changes [e.g., Kepko et al., 2002], solar wind discontinuities [Allan et al., 1986; Wright, 1994], solar wind buffeting [Wright and Rickard, 1995], sudden impulses…”
Magnetic Pulsations: Their Sources and Relation to Solar Wind and Geomagnetic Activity (2005, background): “Kepko et al. (2002) show that the spectrum of the dynamic pressure has multiple peaks at frequencies including f=0.4, 0.7, 1.0, and 1.3 mHz.”
Global characteristics of electromagnetic ion cyclotron waves: Occurrence rate and its storm dependence (2013, background): “…by the solar wind, due to the compression of the magnetosphere caused by variations of the solar wind dynamic pressure [e.g., Mathie and Mann, 2000; Kepko, 2002] and the Kelvin-Helmholz instabilities predominantly on the flank side of the magnetopause [e.g., Chen and Hasegawa, 1974; Southwood,…”