On the solar wind control of Pc5 ULF pulsation power at mid‐latitudes: Implications for MeV electron acceleration in the outer radiation belt

By R. A. Mathie, Ian R. Mann. 2001

171 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/5ff9ef42c90aa80f4aeb97673ae0ac884fe4b7be

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In Astronomy and Astrophysics

1. R. Thorne
2. Wen Li
3. Nigel P. Meredith
4. Y. Shprits
5. R. Horne
6. M. Hudson
7. Binbin Ni
8. J. Fennell

In Molecular Biology

1. Wen Li
2. R. Thorne
3. J. Borovsky
4. M. Denton
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7. Nigel P. Meredith
8. Seth G. Claudepierre

Citations in the corpus

• Radial diffusion and MHD particle simulations of relativistic electron transport by ULF waves in the september 1998 storm (2006, result): “The power is higher during the main phase and in the beginning of recovery phase, and increases with L, which is consistent with observations [ Mathie and Mann, 2000, 2001 ].”
• Earth's Van Allen Radiation Belts: From Discovery to the Van Allen Probes Era (2019, methodology): “Perry et al. (2005) modeled nonequatorially mirroring electrons, incorporating L and frequency dependence of the wave power based on observations (Bloom & Singer, 1995; Mathie & Mann, 2001), finding the largest diffusion rate for equatorially mirroring electrons.”
• The interaction of ultra-low-frequency pc3-5 waves with charged particles in Earth’s magnetosphere (2017, background): “In general, inner-magnetosphere wave–particle interactions are affected by VLF waves (Brice 1964; Kennel and Petschek 1966; Lyons and Thorne 1970; Lyons et al. 1972; Abel and Thorne 1998a, b) and ULF waves (Southwood and Kivelson 1981, 1982; Mathie and Mann 2001; O’Brien et al. 2003).”
• Energization of relativistic electrons in the presence of ULF power and mev microbursts: Evidence for dual ULF and VLF acceleration (2003, result): “Similar results for the dawn sector power have been found in previous studies [e.g., Mathie and Mann, 2000b, 2001].”
• Space Weather Effects in the Earth’s Radiation Belts (2018, background): “It has been long recognized that energetic particles at geosynchronous Earth orbit (GEO) are modulated by solar wind forcing (e.g., Paulikas and Blake 1979; Baker et al. 1979, 1986, 1990; Blake et al. 1997; Reeves 1998; Mathie and Mann 2001; O’Brien et al. 2001; Li, 2001, 2004; Li et al. 2005, 2011;”
• The Upgraded CARISMA Magnetometer Array in the THEMIS Era (2008, background): “…pulses, buffeting, as well as the KelvinHelmholtz instability (KHI) at the magnetopause (see the schematic in Figure 5.1.2) have all been proposed as drivers for cavity/waveguide modes (e.g. Allan et al. 1986; Mann et al. 1999, 2002; Mann and Wright 1999; Mathie and Mann 2001; Rae et al. 2005).”
• Solar wind driving of magnetospheric ULF waves: Pulsations driven by velocity shear at the magnetopause (2008, methodology): “Note that this quantity is different from the total power (TP) that is often used in ULF studies [e.g., Engebretson et al., 1998; Mathie and Mann, 2001]:”
• Differences between CME‐driven storms and CIR‐driven storms (2006, methodology): “The amplitude of Pc5 oscillations in the magnetosphere is proportional to the solar wind velocity [Engebretson et al., 1998; Mathie and Mann, 2001].”