Source characteristics of ELF/VLF chorus

By D. Lauben, Umran S. Inan, T. Bell, Donald A. Gurnett. 2002

149 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/6c9389d06ebcd9244f0238d26b094c67e1c80b65

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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. Danny Summers

In Geophysics

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

In Molecular Biology

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

Citations in the corpus

• Computer simulation of chorus wave generation in the Earth's inner magnetosphere (2007, background): “They have also revealed that the source region of whistler-mode chorus is close to the magnetic equator at the outside of the plasmapause [Lauben et al., 2002; Inan et al., 2004].”
• Modeling the propagation characteristics of chorus using CRRES suprathermal electron fluxes (2007, background): “…the dayside [Tsurutani and Smith, 1977] but recent studies of Poynting flux show that even though wave power maximises at high latitudes on the dayside, the propagation direction is uniformly away from the equator at all MLT [LeDocq et al., 1998; Lauben et al., 2002; Santolik et al., 2004, 2005].”
• Modeling the evolution of chorus waves into plasmaspheric hiss (2011, background): “…of values, from predominantly field aligned [Burton and Holzer, 1974; Goldstein and Tsurutani, 1984; Hayakawa et al., 1984; Santolik et al., 2003] to ring‐like [Santolik et al., 2009] and oblique [Lefeuvre and Helliwell, 1985; Hayakawa et al., 1990; Lauben et al., 2002; Tsurutani et al., 2008].”
• Statistics of whistler mode waves in the outer radiation belt: Cluster STAFF‐SA measurements (2013, background): “[21] Chorus waves are usually assumed to be generated in the close vicinity of the magnetic equator [Lauben et al., 2002; Parrot et al., 2003; Santolík et al., 2004, 2005].”
• Corotating solar wind streams and recurrent geomagnetic activity: A review (2006, unknown): “It is believed that the frequency ‘‘gap’’ is due to Landau absorption [Tsurutani and Smith, 1974; Coroniti et al., 1984; Lauben et al., 2002; see also Horne et al., 2003].”
• Nonlinear mechanisms of lower-band and upper-band VLF chorus emissions in the magnetosphere (2009, background): “[2] Coherent electromagnetic waves called chorus emissions have been frequently observed in the inner magnetosphere [e.g., Tsurutani and Smith, 1974; Anderson and Kurth, 1989; Lauben et al., 1998, 2002; Santolik et al., 2003; Santolik, 2008; Kasahara et al., 2009].”
• Oblique propagation of whistler mode waves in the chorus source region (2009, background): “Direct or indirect observations of wave vector directions in other cases [e.g., Lefeuvre and Helliwell, 1985; Hayakawa et al., 1990; Lauben et al., 2002; Tsurutani et al., 2008] however suggest that large wave vector angles with respect to the terrestrial magnetic field can also be encountered.”
• Global model of lower band and upper band chorus from multiple satellite observations (2012, background): “Chorus is generated outside the plasmapause near the geomagnetic equator [LeDocq et al., 1998; Lauben et al., 2002; Santolík et al., 2004, 2005] by cyclotron resonant interaction with suprathermal electrons [Katoh and Omura, 2007; Omura et al., 2008; Li et al., 2008, 2009a] injected into the inner…”
• The dual role of ELF/VLF chorus waves in the acceleration and precipitation of radiation belt electrons (2007, methodology): “Ray tracing combined with direction finding also indicates that chorus may be generated at the Gendrin angle (or high wave normal angles) near the source region (Lauben et al., 2002; Parrot et al., 2003) which could be related to its unidirectional propagation and twobanded structure (Bortnik et al.”
• THEMIS analysis of observed equatorial electron distributions responsible for the chorus excitation (2010, background): “However, analyses of wave normal angles for upper‐ band chorus have led to widely diverse results, ranging from essentially field‐aligned [e.g., Lauben et al., 2002] to highly oblique with wave normal angles close to the resonance cone [e.g., Hayakawa et al., 1984; Muto et al., 1987].”
• Resonant scattering of plasma sheet electrons leading to diffuse auroral precipitation: 2. Evaluation for whistler mode chorus waves (2011, background): “…2) which varies with magnetic latitude interval and is basically representative of the theoretical simulations and observations [e.g., Hayakawa et al., 1984; Hospodarsky et al., 2001; Lauben et al., 2002; Bortnik et al., 2006; Li et al., 2008, 2009b; Breneman et al., 2009; Haque et al., 2010].”