Three‐dimensional diffusion simulation of outer radiation belt electrons during the 9 October 1990 magnetic storm

By J. Albert, Nigel P. Meredith, R. Horne. 2009

171 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/59d99b26b672d167b628aa26bd792668714fd751

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. Wen Li
4. R. Horne
5. Binbin Ni
6. Jacob Bortnik
7. Y. Shprits
8. S. Glauert

In Molecular Biology

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

Citations in the corpus

• Event‐specific chorus wave and electron seed population models in DREAM3D using the Van Allen Probes (2014, methodology): “Typically, for the calculation of the pitch angle/momentum diffusion coefficients in the 3-D diffusion codes, empirical wave distributions derived from a statistical wave database are used [Albert et al., 2009; Tu et al., 2013].”
• Origin of energetic electron precipitation >30 keV into the atmosphere (2010, methodology): “, 2005] and used in global simulation models [Varotsou et al., 2005, 2008; Fok et al., 2008; Albert et al., 2009].”
• Three‐dimensional electron radiation belt simulations using the BAS Radiation Belt Model with new diffusion models for chorus, plasmaspheric hiss, and lightning‐generated whistlers (2014, methodology): “Brautigam and Albert [2000] presented radial diffusion rates parameterized by the geomagnetic index Kp that have since been widely used in radiation belt modeling codes [e.g., Varotsou et al., 2005; Albert et al., 2009; Subbotin and Shprits, 2009].”
• Modeling radiation belt electron dynamics during GEM challenge intervals with the DREAM3D diffusion model (2013, background): “, 2007], and 3D diffusion models that include all three types of diffusion [Albert et al., 2009; Su et al., 2011; Subbotin et al., 2011; Kim et al., 2012].”
• 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‐”
• Radiation belt electron acceleration by chorus waves during the 17 March 2013 storm (2014, methodology): “This study, together with other previous studies simulating electron acceleration events [e.g., Horne et al., 2005a; Albert et al., 2009; Glauert et al., 2014; Shprits et al., 2009; Xiao et al., 2009; Su et al., 2010; Thorne et al., 2013; Tu et al., 2014; Turner et al., 2014], suggests that the…”
• Resonant scattering of plasma sheet electrons leading to diffuse auroral precipitation: 2. Evaluation for whistler mode chorus waves (2011, unknown): “…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 al., 2009, 2010; Subbotin and Shprits, 2009; Subbotin et al., 2010].”
• Earth's Van Allen Radiation Belts: From Discovery to the Van Allen Probes Era (2019, background): “Moreover, recent multidimensional diffusion simulations reproduced the main features of observed radiation belt electron dynamics (Albert et al., 2009; Drozdov et al., 2015; Fok et al., 2008; Fok et al., 2014; Glauert et al., 2014; W. Li, Ma, et al., 2016; Ma et al., 2018; Shprits et al., 2009;…”
• Global model of lower band and upper band chorus from multiple satellite observations (2012, methodology): “[7] There are several dynamic global models of the radiation belts which are based on diffusion models [e.g., Varotsou et al., 2005, 2008; Fok et al., 2008; Subbotin et al., 2010; Albert et al., 2009].”
• The Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) on RBSP (2013, background): “…multidimensional diffusion models (Jordanova and Miyoshi 2005; Jordanova et al. 2008; Fok et al. 2008; Tao et al. 2008, 2009; Varotsou et al. 2008; Albert et al. 2009; Shprits et al. 2009; Subbotin and Shprits 2009; Tu et al. 2009) are required to differentiate between the different source and…”
• Radiation belt dynamics: The importance of wave‐particle interactions (2010, methodology): “The importance of local stochastic acceleration by chorus, relative to acceleration associated with inward radial diffusion, has recently been demonstrated by modeling with 3D diffusion codes [Albert et al., 2009; Varotsou et al., 2008; Shprits et al., 2009b].”
• Three-dimensional simulations of outer radiation belt electron dynamics including cross-diffusion terms (2010, methodology): “new variables to allow cross diffusion terms vanishing in the 2‐D or 3‐D diffusion equation [Albert and Young, 2005; Albert et al., 2009], adopted a Monte Carlo method [Tao et al.”