Evaluation of quasi-linear diffusion coefficients for whistler mode waves in a plasma with arbitrary density ratio

By J. Albert. 2005

200 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/4a33d998c98a0ed34fa919588788d1fd1751cbdb

How researchers see this paper

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

In Astronomy and Astrophysics

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

In Nuclear and High Energy Physics

1. R. Thorne
2. Y. Shprits
3. R. Horne
4. I. Usoskin
5. Wen Li
6. Binbin Ni
7. Nigel P. Meredith
8. G. Kovaltsov

Citations in the corpus

• Bounce‐averaged diffusion coefficients for field‐aligned chorus waves (2006, methodology): “Horne et al. [2005] and Albert [2005] used the full cold plasma dispersion relationship to estimate bounce-averaged diffusion coefficients, assuming a Gaussian spread of wave power spectral density in both frequency and wave normal angle.”
• Radiation belt dynamics: The importance of wave‐particle interactions (2010, background): “tivistic energies on timescale comparable to a day [Albert, 2005; Horne et al., 2005a].”
• Dependence of the quasi‐linear scattering rates on the wave normal distribution of chorus waves (2009, methodology): “The code uses a formulation similar to that of Glauert and Horne [2005] and Albert [2005] .”
• THEMIS analysis of observed equatorial electron distributions responsible for the chorus excitation (2010, background): “More comprehensive information on the injected electron phase space density (PSD) and anisotropy over the entire inner magnetosphere is required to understand the global distribution of chorus excitation and its effect on energetic radiation belt electrons [Meredith et al., 2001; Summers et al., 200”
• Modeling of outer radiation belt electrons by multidimensional diffusion process (2009, background): “density approximation for the dispersion relation in the whistler mode wave frequency range [Lyons, 1974; Albert, 2005].”
• Particle Dynamics in the Earth's Radiation Belts: Review of Current Research and Open Questions (2020, background): “Aside fromVan Allen Probes, what other reliable observations can be brought to bear on the subject of electron loss from the inner zone or, more generally, at low L‐shells?”
• Calculation of pitch angle and energy diffusion coefficients with the PADIE code (2005, methodology): “A similar code is being developed elsewhere, but as far as we are aware, it is restricted to whistler mode waves [ Albert, 2005 ].”
• Parameterization of radiation belt electron loss timescales due to interactions with chorus waves (2007, result): “For E > 100 keV the scattering rates are higher for the lower energy particles, consistent with previous studies [e.g., Horne et al., 2005a; Albert, 2005].”
• Earth's Van Allen Radiation Belts: From Discovery to the Van Allen Probes Era (2019, background): “However, Ma, Li, et al. (2016b) showed that the acceleration timescale based on the statistical magnetosonic wave distribution is typically longer (approximately several days) than that of chorus waves (less than a day; Albert, 2005; Horne et al., 2005; Thorne et al., 2013a).”
• Timescale for MeV electron microburst loss during geomagnetic storms (2005, methodology): “Diffusion codes have recently been developed [Horne et al., 2003a, 2005; Albert, 2005; Glauert and Horne, 2005] to evaluate the bounce-averaged rate of pitch angle scattering.”
• Multidimensional quasi‐linear diffusion of radiation belt electrons (2005, background): “It has been argued that the condition fpe fce enables storm-time enhanced whistler mode chorus to drive rapid electron acceleration [Summers et al., 1998; Horne et al., 2003, 2005; Albert, 2005], which could account for the energized population.”
• Dynamics of the Earth’s Particle Radiation Environment (2009, background): “A number of new pitch angle diffusion studies (e.g., Albert 2005; Ni et al. 2008) and new global radiation belt models have been developed (e.g., Miyoshi et al. 2006; Fok et al. 2008; Varotsou et al. 2008), which show that electron acceleration by whistler mode chorus waves is a key physical…”
• Dynamic evolution of energetic outer zone electrons due to wave‐particle interactions during storms (2007, background): “Most of the previous studies concentrated on computing only pitch angle and energy scattering rates by chorus [ Albert, 2005; Horne et al., 2005], EMIC [Summers and Thorne, 2003; Summers, 2005], or hiss waves [Meredith et al., 2006].”
• Outward radial diffusion driven by losses at magnetopause (2006, background): “Theoretical estimates of the scattering rates indicate that losses due to chorus waves occur throughout the outer radiation belt [Albert, 2005; Horne et al., 2005a; Thorne et al., 2005b].”
• Evolution of electron fluxes in the outer radiation belt computed with the VERB code (2009, methodology): “The code uses a formulation of Glauert and Horne [2005] and Albert [2005] .”