Evolution of electron fluxes in the outer radiation belt computed with the VERB code

By Y. Shprits, D. Subbotin, Binbin Ni. 2009

216 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/5ee5e30513bfeb32b00d443c4e1ee97108f83c34

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. Wen Li
3. Nigel P. Meredith
4. R. Horne
5. Y. Shprits
6. Jacob Bortnik
7. Binbin Ni
8. J. Fennell

In Molecular Biology

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

Citations in the corpus

• On the storm‐time evolution of relativistic electron phase space density in Earth's outer radiation belt (2013, background): “…and 2- and 3-dimensional diffusion modeling for stochastic wave-particle interactions with chorus [e.g., Horne et al., 2005; Li et al., 2007; Shprits et al., 2009b], are predominantly scattered up in energy and away from the loss cone; such diffusion promotes rapid energization over loss to…”
• The Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) on RBSP (2013, background): “…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 loss processes.”
• Statistical properties of plasmaspheric hiss derived from Van Allen Probes data and their effects on radiation belt electron dynamics (2015, background): “…a Gaussian wave frequency spectrum with a peak frequency of ~550Hz and frequency bandwidth of ~300Hz has been frequently adopted over the range of wave frequencies between 100Hz and 2 kHz [Lyons et al., 1972; Summers et al., 2007; Shprits et al., 2009; Thorne et al., 2013; Ni et al., 2013, 2014].”
• Resonant scattering of plasma sheet electrons leading to diffuse auroral precipitation: 2. Evaluation for whistler mode chorus waves (2011, background): “…been recognized due to its dual role in both the acceleration and precipitation of radiation belt energetic electrons [e.g., Horne and Thorne, 2003; Horne et al., 2005a; Thorne et al., 2005a; Albert, 2004, 2007; Bortnik and Thorne, 2007; Summers et al., 2007a, 2007b; Shprits et al., 2008, 2009b].”
• 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].”
• Particle Dynamics in the Earth's Radiation Belts: Review of Current Research and Open Questions (2020, background): “D code (e.g., Subbotin & Shprits, 2009; Shprits et al., 2009; Subbotin et al., 2010, 2011; Kim et al., 2011, Kim et al., 2012; Drozdov et al., 2015) recently extended to a 4‐”
• Radiation belt electron acceleration by chorus waves during the 17 March 2013 storm (2014, result): “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 chor”