Evolution and characteristics of global Pc5 ULF waves during a high solar wind speed interval

By I. J. Rae, E. Donovan, Ian R. Mann, F. Fenrich, C. Watt, D. Milling, M. Lester, B. Lavraud, J. Wild, H. Singer and 2 more. 2005

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The Upgraded CARISMA Magnetometer Array in the THEMIS Era (2008, methodology): “Multi-point studies with THEMIS can examine the waves in the magnetosphere at the times of well-defined CARISMA observed FLRs, as well as the nature of fluctuations at the magnetopause (e.g. Mann et al. 2002; Rae et al. 2005) and even in the sheath and solar wind, especially on the flanks.”
The interaction of ultra-low-frequency pc3-5 waves with charged particles in Earth’s magnetosphere (2017, background): “H instability, waves generated by this instability show minimum activity around noon near the subsolar stagnation region compared with the dawn and dusk sector (e.g., Anderson et al. 1990; Zhu and Kivelson 1991; Lessard et al. 1999; Hudson et al. 2004; Rae et al. 2005; Takahashi and Ukhorsky 2007).”
Review of the accomplishments of mid-latitude Super Dual Auroral Radar Network (SuperDARN) HF radars (2019, background): “Critically, such waves can be observed either in ionospheric scatter (Rae et al. 2005), in ground scatter (Ponomarenko et al. 2003), or in artificially stimulated ionospheric scatter (Yeoman et al. 1997).”