Parameterization of radiation belt electron loss timescales due to interactions with chorus waves

By Y. Shprits, Nigel P. Meredith, R. Thorne. 2007

141 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/4fec4f4ced8115935b14316bc1dae0dfe226441c

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In Astronomy and Astrophysics

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

In Geophysics

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

Citations in the corpus

• Oblique propagation of whistler mode waves in the chorus source region (2009, methodology): “where P and S are the parameters of Stix [1992] calculated using f, fce, and fp.”
• Evolution of electron fluxes in the outer radiation belt computed with the VERB code (2009, methodology): “A11209 following Shprits et al. [2007a] . In this case the pronounced peak in fluxes is formed only after approximately 1 day into the recovery phase of the storm.”
• Dynamic evolution of energetic outer zone electrons due to wave‐particle interactions during storms (2007, methodology): “The complete sets of wave properties used in our simulation (listed in Table 1) are based on previous observational studies [Horne et al., 2005; Meredith et al., 2004, 2006; Loto’aniu et al., 2006; Sheeley et al., 2001; Spasojevic ´e t al., 2003; Shprits et al., 2007 ].”
• Three-dimensional simulations of outer radiation belt electron dynamics including cross-diffusion terms (2010, background): “04l [pT] within l ≤ 35° [Li et al., 2007; Shprits et al., 2007].”
• Modeling of outer radiation belt electrons by multidimensional diffusion process (2009, result): “Therefore, on the basis of the previous results [Li et al., 2007; Shprits et al., 2007], we choose the”
• The Geomagnetic Kp Index and Derived Indices of Geomagnetic Activity (2021, background): “, McIlwain, 1986), lower band chorus/VLF wave activity (e.g., Agapitov et al., 2015; Shprits et al., 2007) and ultra low frequency (ULF) wave activity (e.”
• Resonant scattering of plasma sheet electrons leading to diffuse auroral precipitation: 2. Evaluation for whistler mode chorus waves (2011, unknown): “…1998b; Horne et al., 2003, 2005a, 2005b; Thorne et al., 2005a, 2005b, 2007, 2010;Glauert and Horne, 2005; Summers, 2005; Varotsou et al., 2005, 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,…”
• Modeling radiation belt electron dynamics during GEM challenge intervals with the DREAM3D diffusion model (2013, background): “The contributing waves include chorus, considered effective outside the plasmasphere [O’Brien et al., 2004; Thorne et al., 2005; Shprits et al., 2007], plasmaspheric hiss 1Science and Applications Group, Los Alamos National Laboratory, Los Alamos, New Mexico, USA.”
• THEMIS analysis of observed equatorial electron distributions responsible for the chorus excitation (2010, background): “Upper‐ band chorus tends to have a peak intensity near 0.55 fce, while lower‐band chorus peaks at 0.3–0.4 fce on the nightside and at 0.2–0.3 fce on the dayside [e.g., Bortnik et al., 2007; Shprits et al., 2007].”