Simulation of the outer radiation belt electrons near geosynchronous orbit including both radial diffusion and resonant interaction with Whistler‐mode chorus waves
By Athena Varotsou, D. Boscher, S. Bourdarie, R. Horne, S. Glauert, Nigel P. Meredith. 2005
148 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/fedafa0e5d499f1993116aaa539dc5d08b672e7d
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Citations in the corpus
- Timescales for radiation belt electron acceleration and loss due to resonant wave-particle interactions: 1. Theory (2007, background): “…due to cyclotron resonance with chorus waves is a viable mechanism for generating relativistic electrons (>1 MeV) in the outer zone during storms [Summers et al., 1998, 2002, 2004a, 2004b; Roth et al., 1999; Summers and Ma, 2000; Horne et al., 2005a; Thorne et al., 2005a; Varotsou et al., 2005].”
- Electron acceleration in the Van Allen radiation belts by fast magnetosonic waves (2007, background): “Since chorus waves are very effective in producing MeV electrons [Varotsou et al., 2005], we sug-”
- Outward radial diffusion driven by losses at magnetopause (2006, background): “In this case, radial diffusion works as a loss outside of the peak in phase space density and will accelerate electrons inside of the peak [Varotsou et al., 2005].”
- Modeling the propagation characteristics of chorus using CRRES suprathermal electron fluxes (2007, background): “…et al., 2005a, 2005b; Spasojevic and Inan, 2005; Meredith et al., 2002a, 2002b, 2003b; Miyoshi et al., 2003; Lyons et al., 2005; Smith et al., 2004; Varotsou et al., 2005; Shprits et al., 2006] playing a dual role in both the precipitation and acceleration of radiationbelt electrons [Horne and…”
- Resonant scattering of plasma sheet electrons leading to diffuse auroral precipitation: 2. Evaluation for whistler mode chorus waves (2011, unknown): “…2008; Abel and Thorne, 1998a, 1998b; Horne et al., 2003, 2005a, 2005b; Thorne et al., 2005a, 2005b, 2007, 2010;Glauert 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;…”
- Dependence of the quasi‐linear scattering rates on the wave normal distribution of chorus waves (2009, background): “Pitch angle and energy diffusion codes accounting for mixed diffusion [Albert and Young, 2005; Tao et al., 2008], convective codes including pitch angle and/or energy diffusion [Jordanova et al., 2003; Jordanova and Miyoshi, 2005; Miyoshi et al., 2006; Fok et al., 2008], and three-dimensional diffus”
- Origin of energetic electron precipitation >30 keV into the atmosphere (2010, methodology): “The wave parameters are based on those used before for studying lower‐band whistler mode chorus, and which were obtained from analyzing whistler mode data [Meredith et al., 2002; Horne et al., 2005] and used in global simulation models [ Varotsou et al., 2005, 2008; Fok et al., 2008; Albert et al., ”
- Theory and simulation of the generation of whistler‐mode chorus (2008, unknown): “In particular, energy diffusion due to electron gyroresonance with chorus is a key mechanism for generating relativistic electrons in the region 3 < L < 5 outside the plasmasphere during geomagnetic storms or periods of prolonged substorm activity [Summers et al., 1998, 2002, 2004a, 2004b, 2007a, 20”
- Radiation Belt Environment model: Application to space weather nowcasting (2008, background): “Varotsou et al. [2005] and Horne et al. [2006] combined radial diffusion with acceleration and loss due to whistler mode chorus waves and confirmed that wave acceleration by whistler mode chorus is an important acceleration mechanism in the outer radiation belt.”
- Modeling of outer radiation belt electrons by multidimensional diffusion process (2009, background): “Li et al. [2007] presented solutions of a 2-D code (by ignoring cross diffusion terms) to examine effects of acceleration and loss due to resonant interaction with field-aligned propagated whistler mode chorus, hiss and electromagnetic ion cyclotron (EMIC) waves. Varotsou et al.[2005] solved a 3-D ”
- Evolution of electron fluxes in the outer radiation belt computed with the VERB code (2009, methodology): “In its formulations the VERB code is rather similar to the latest versions of the Salammboˆ diffusion code [ Varotsou et al., 2005, 2008 ], which solves for the evolution of the PSD in terms of momentum, pitch angle, and radial distance.”
- Energetic outer zone electron loss timescalesduring low geomagnetic activity (2006, background): “... the reviews by Li and Temerin [2001], Horne [2002], and Friedel et al. [2002]), recent experimental and modelling work suggests that the acceleration is caused by a combination of enhanced inward radial diffusion driven by ULF waves [e.g., Elkington et al., 1999; Liu et al., 1999; Hudson et al.,”
- Relativistic turning acceleration of resonant electrons by coherent whistler mode waves in a dipole magnetic field (2007, background): “A physical mechanism that can account for the storm-time generation of relativistic electrons is cyclotron resonance with whistler mode chorus waves outside the plasmasphere [Summers et al., 1998, 2002, 2004; Roth et al., 1999; Summers and Ma, 2000; Meredith et al. ,2 002;Albert, 2002; Miyoshi et al”
- Particle Dynamics in the Earth's Radiation Belts: Review of Current Research and Open Questions (2020, background): “…codes are the ONERA Salammbô code (e.g., Beutier & Boscher, 1995; Bourdarie et al., 1996, 2000, 2005; Pugacheva et al., 2000; Beutier et al., 2005; Varotsou et al., 2005, 2008; Maget et al., 2015; Herrera et al., 2016), the British Antarctic Survey (BAS) Radiation Belt Code (e.g., Glauert et…”
- Electron scattering by whistler-mode ELF hiss in (2008, unknown): “…plasmaspheric plumes [Summers et al., 1998, 2002, 2004, 2007b; Horne and Thorne, 1998; Roth et al., 1999; Summers and Ma, 2000; Meredith et al., 2002, 2003a; Miyoshi et al., 2003; Horne et al., 2005a, 2005b; Varotsou et al., 2005; Omura and Summers, 2006; Shprits et al., 2006b; Li et al., 2007].”
- Timescales for radiation belt electron acceleration and loss due to resonant wave‐particle interactions: 2. Evaluation for VLF chorus, ELF hiss, and electromagnetic ion cyclotron waves (2007, background): “, 1999], the quasi-linear diffusion formalism [Summers and Ma, 2000; Summers et al., 2002, 2004b; Miyoshi et al., 2003; Horne et al., 2005a, 2005b; Varotsou et al., 2005; Shprits et al., 2006a], and a self-consistent wave-particle simulation code [Katoh and Omura, 2004] confirm that electron acceler”