Diffuse auroral electron scattering by electron cyclotron harmonic and whistler mode waves during an isolated substorm

By R. Horne, R. Thorne, Nigel P. Meredith, R. R. Anderson. 2003

186 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/2d12ba739a7959aaf38e3a28ffb847f52bfbb4c8

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. Jacob Bortnik
4. R. Horne
5. Nigel P. Meredith
6. Binbin Ni
7. Y. Shprits
8. V. Angelopoulos

In Geophysics

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

Citations in the corpus

• Resonant scattering of plasma sheet electrons leading to diffuse auroral precipitation: 2. Evaluation for whistler mode chorus waves (2011, background): “…whistler mode chorus waves have received the most extensive investigations [e.g., Kennel et al., 1970; Lyons, 1974c; Inan et al., 1992; Villalón and Burke, 1995; Horne and Thorne, 2000; Horne et al., 2003; Ni et al., 2008; Meredith et al., 2000, 2009; Su et al., 2009, 2010; Thorne et al., 2010].”
• Global distributions of suprathermal electrons observed on THEMIS and potential mechanisms for access into the plasmasphere (2010, background): “…and Bortnik et al. [2007], possibly due to pitch angle scattering by chorus waves and electrostatic Electron Cyclotron Harmonic (ECH) waves [e.g., Horne et al., 2003; Ni, et al., 2008; Su et al., 2009; Thorne et al., 2010] and magnetopause shadowing [e.g., Li et al., 1997; Desorgher et al.,…”
• THEMIS analysis of observed equatorial electron distributions responsible for the chorus excitation (2010, background): “Although the excitation mechanism for upper‐band chorus remains debatable [e.g., Hashimoto and Kimura, 1981; Horne et al., 2003a ], it has been generally accepted that lower‐band chorus waves can be generated through a cyclotron resonance with anisotropic electrons with energies between a few and t”
• Modeling of outer radiation belt electrons by multidimensional diffusion process (2009, background): “Electromagnetic waves can also produce pitch angle scattering of electrons [Summers et al., 1998; Horne et al., 2003b; Summers and Thorne, 2003], yielding precipitation loss into the atmosphere and ozone destruction by change of atmospheric chemistry [Thorne, 1977; Callis et al., 1998].”
• Survey of upper band chorus and ECH waves: Implications for the diffuse aurora (2009, background): “[e.g., Belmont et al., 1983, 1984; Lyons, 1984; Roeder and Koons, 1989; Johnstone et al., 1993; Meredith et al., 1999, 2000; Horne and Thorne, 2000; Horne et al., 2003; Ni et al., 2008].”
• The Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) on RBSP (2013, background): “2010b), while the electron distributions can excite whistler-mode waves (e.g., Kennel and Thorne 1967; Horne et al. 2003).”
• Resonant scattering of plasma sheet electrons by whistler‐mode chorus: Contribution to diffuse auroral precipitation (2008, background): “Detailed quasi-linear scattering rates, based on observed wave spectral properties, demonstrated that ECH waves are capable of causing strong diffusion scattering of electrons ( 1 keV) near the loss cone [Horne et al., 2003].”
• Three-dimensional simulations of outer radiation belt electron dynamics including cross-diffusion terms (2010, background): “Meanwhile, plasma waves can cause precipitation loss of energetic electrons into the atmosphere by pitch‐angle scattering [ Horne et al., 2003b; Summers and Thorne, 2003; Xiao et al., 2009b], yielding ozone destruction by change of atmospheric chemistry [Thorne, 1977; Callis et al., 1998].”