Electron scattering by whistler-mode ELF hiss in

By Danny Summers, Binbin Ni, Nigel P. Meredith, R. Horne, R. Thorne, Mark B. Moldwin, R. R. Anderson. 2008

202 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/0b391ee105b217eb0aae79936be32d408fa508cb

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In Astronomy and Astrophysics

1. R. Thorne
2. Nigel P. Meredith
3. Wen Li
4. R. Horne
5. Binbin Ni
6. Y. Shprits
7. Jacob Bortnik
8. S. Glauert

In Geophysics

1. R. Thorne
2. Nigel P. Meredith
3. Wen Li
4. R. Horne
5. Binbin Ni
6. Jacob Bortnik
7. Y. Shprits
8. S. Glauert

Citations in the corpus

• Radiation belt electron acceleration by chorus waves during the 17 March 2013 storm (2014, background): “…loss due to the open drift trajectory [Chen et al., 2003], pitch angle scattering by hiss in plumes, which is more effective for lower energies [Li et al., 2007; Summers et al., 2008; Ni et al., 2013], and radial diffusion process [e.g., Perry et al., 2005; Turner et al., 2012], as discussed above.”
• Resonant scattering of plasma sheet electrons leading to diffuse auroral precipitation: 2. Evaluation for whistler mode chorus waves (2011, unknown): “…and Horne, 2005; Summers, 2005; Varotsou et al., 2005, 2008; Shprits et al., 2006b, 2007, 2008, 2009a, 2009b; Summers et al., 2007a, 2007b; Summers et al., 2008; Fok et al., 2008; Tao et al., 2008, 2009, 2011; Shprits and Ni, 2009; Albert et al., 2009; Xiao et al., 2009, 2010; Su et…”
• Particle Dynamics in the Earth's Radiation Belts: Review of Current Research and Open Questions (2020, background): “Whistler mode hiss waves are also observed in high‐density plumes outside the plasmasphere (Chan & Holzer, 1976; Summers et al., 2008) and the characterization of their properties and their effect outside the plasmasphere is ongoing (Woodroffe et al., 2017; Su et al., 2018; Shi et al., 2019; Li et…”
• Origin of energetic electron precipitation >30 keV into the atmosphere (2010, background): “During active conditions, equatorial hiss (∣MLAT∣ Summers et al., 2008 ], however this tends to be confined to the postnoon sector.”
• Radiation belt dynamics: The importance of wave‐particle interactions (2010, background): “Hiss is also observed in plasmaspheric plumes during a storm, and such waves are sufficiently intense (Bw ∼ 100 pT) to contribute significantly to the scattering loss of outer zone electrons [Summers et al., 2008].”
• Statistical properties of plasmaspheric hiss derived from Van Allen Probes data and their effects on radiation belt electron dynamics (2015, background): “…is a structureless and broadband whistler mode emission typically observed inside the plasmasphere [Dunckel and Helliwell, 1969; Thorne et al., 1973; Meredith et al., 2004] and high-density plumes in the Earth’s magnetosphere [Chan and Holzer, 1976; Parrot and Lefeuvre, 1986; Summers et al., 2008].”
• Plasmaspheric Density Structures and Dynamics: Properties Observed by the CLUSTER and IMAGE Missions (2009, background): “Later satellite measurements revealed concentrations of cross-field density irregularities in the vicinity of the plasmapause, for example with the LANL geosynchronous satellites (Moldwin et al. 1995) or the CRRES spacecraft (Fung et al. 2000).”
• Modeling the evolution of chorus waves into plasmaspheric hiss (2011, background): “In addition, PH is often observed in plumes, which could play a further role in shaping outer radiation belt dynamics [Summers et al., 2008].”
• Relativistic electron loss timescales in the slot region (2009, unknown): “plumes [Chan and Holzer, 1976; Cornilleau-Wehrlin et al., 1978; Parrot and Lefeuvre, 1986; Summers et al., 2008 ].”
• Global model of lower band and upper band chorus from multiple satellite observations (2012, background): “…et al., 1969; Thorne et al., 1973] and plasmaspheric plumes [Chan and Holzer, 1976; Cornilleau-Wehrlin et al., 1978; Parrot and Lefeuvre, 1986; Summers et al., 2008] and lightning generated whistlers are largely confined to the plasmasphere [Carpenter et al., 1968, 1969; Platino et al., 2005].”
• Earth's Van Allen Radiation Belts: From Discovery to the Van Allen Probes Era (2019, background): “…pitch angle scattering loss driven by whistler mode waves in plumes could be stronger than plasmaspheric hiss, particularly at lower energy (W. Li et al., 2019), suggesting their potential importance in energetic electron loss process (e.g., Summers et al., 2008; W. Zhang, Fu, et al., 2018).”