Multidimensional quasi‐linear diffusion of radiation belt electrons

By J. Albert, S. L. Young. 2005

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View Paper: https://www.semanticscholar.org/paper/3eaa2b2fdd58b411086fb2fc65e10a751a652e27

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In Astronomy and Astrophysics

Citations in the corpus

Particle Dynamics in the Earth's Radiation Belts: Review of Current Research and Open Questions (2020, background): “D), the radiation belt code of the Space Vehicles Directorate of the U.S. Air Force Research Laboratory (AFRL) (e.g., Albert, 2005, 2008b; Albert et al., 2009; Albert & Young, 2005; Selesnick, Albert, & Starks, 2013), the LANL Dynamic Radiation Environment Assimilation Model (DREAM) 1‐”
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 diff”
Modeling of outer radiation belt electrons by multidimensional diffusion process (2009, result): “Meanwhile, we have performed some numerical tests for diffusion coefficients, and evolution of phase space density by using the same parameters as those in the previous work [ Albert and Young, 2005; Li et al., 2007; Summers et al., 2007b] and found good agreements with those previous results by ta”
Evolution of electron fluxes in the outer radiation belt computed with the VERB code (2009, methodology): “As shown by Albert and Young [2005] , who followed the method described by Schulz and Lanzerotti [1974, pp. 105–106], mixed diffusion does not significantly change electron fluxes at high pitch angles.”
Dynamic evolution of energetic outer zone electrons due to wave‐particle interactions during storms (2007, background): “Added complexity due to the inclusion of oblique waves [e.g., Albert, 2005; Horne et al., 2005], and mixed diffusion terms [ Albert and Young, 2005 ] will be left for future studies.”
Discovery of very large amplitude whistler‐mode waves in Earth's radiation belts (2008, background): “Acceleration of electrons by low amplitude whistler-mode ‘chorus’ waves is currently accepted to be an important process in the outer belt [Summers et al., 1998; Roth et al., 1999; Summers and Ma, 2000; Meredith et al., 2001; Horne and Thorne, 2003; Horne et al., 2005; Albert and Young, 2005].”
Radiation Belt Environment model: Application to space weather nowcasting (2008, background): “important [ Albert and Young, 2005 ], has not been included in the model.”
Three-dimensional simulations of outer radiation belt electron dynamics including cross-diffusion terms (2010, methodology): “In order to prevent this problem, previous work used a transforming technique of new variables to allow cross diffusion terms vanishing in the 2‐ Do r 3 ‐D diffusion equation [ Albert and Young, 2005; Albert et al., 2009], adopted a Monte Carlo method [Tao et al., 2008], or ran a layer code [Tao et”