Dependence of the quasi‐linear scattering rates on the wave normal distribution of chorus waves

By Y. Shprits, Binbin Ni. 2009

174 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/b8cf4e2c6abdc4ba27ba3d62af13eca0a3be8a9e

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. Binbin Ni
7. Jacob Bortnik
8. J. Fennell

In Geophysics

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

Citations in the corpus

• Resonant scattering of outer zone relativistic electrons by multiband EMIC waves and resultant electron loss time scales (2015, methodology): “The Full Diffusion Code [Ni et al., 2008, 2011; Shprits and Ni, 2009] is implemented to compute the quasi-linear bounce-averaged diffusion coefficients in the dipole field for various EMIC wave normal angle distributions.”
• Constructing the global distribution of chorus wave intensity using measurements of electrons by the POES satellites and waves by the Van Allen Probes (2013, methodology): “Based on these assumptions, using the Full Diffusion Code [Ni et al., 2008; Shprits and Ni, 2009], we calculate bounce-averaged pitch angle diffusion coefficients Dαα(E) at the equatorial loss cone, which are subsequently used to infer chorus wave power (Bw 2) in each L-MLT bin.”
• Radiation belt dynamics: The importance of wave‐particle interactions (2010, background): “tribution of chorus is required to accurately evaluate resonant electron energies and quantify the associated rates of scattering [Shprits and Ni, 2009].”
• Evolution of electron fluxes in the outer radiation belt computed with the VERB code (2009, methodology): “Quasi-linear diffusion coefficients are computed with the Full Diffusion Code (FDC)recentlydevelopedattheUniversityofCalifornia,Los Angeles (UCLA); the code is capable of computing resonance scattering rates, including high-order scattering by obliquely propagating waves, which was recently used by ”
• The Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) on RBSP (2013, background): “The wave normal distribution of chorus is required to accurately evaluate resonant electron energies and quantify the associated rates of scattering (Shprits and Ni 2009).”
• Particle Dynamics in the Earth's Radiation Belts: Review of Current Research and Open Questions (2020, methodology): “D diffusion code (e.g., Tao et al., 2011; Li et al., 2014; Li, Ma, et al., 2016; Ma et al., 2015, 2016, 2016, Ma et al., 2017 that incorporates the (UCLA) Full Diffusion Code (e.g., Ni et al., 2008, Ni et al., 2011; Shprits & Ni, 2009) in order to compute diffusion coefficients (similarly to VERB 3‐”
• Resonant scattering of plasma sheet electrons leading to diffuse auroral precipitation: 2. Evaluation for whistler mode chorus waves (2011, methodology): “…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].”
• Radiation belt electron acceleration by chorus waves during the 17 March 2013 storm (2014, methodology): “Drift and bounce averaged diffusion coefficients driven by lower-band chorus waves at L= 4.25 are computed using the UCLA full diffusion code [Ni et al., 2008, 2011; Shprits and Ni, 2009] in a dipole magnetic field model based on the parameters shown in Table 1.”
• Statistics of whistler mode waves in the outer radiation belt: Cluster STAFF‐SA measurements (2013, background): “It results in an increase of the role of higher order cyclotron harmonic resonances and leads to a significant growth of electron pitch angle diffusion rates, especially for low equatorial electron pitch angles [Shprits and Ni, 2009; Artemyev et al., 2012a].”