Oblique propagation of whistler mode waves in the chorus source region
By O. Santolík, Donald A. Gurnett, J. Pickett, J. Chum, N. Cornilleau-Wehrlin. 2009
156 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Geophysics
View Paper: https://www.semanticscholar.org/paper/37014eec276e09549003ddac9074dd0e5dcc6083
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Citations in the corpus
- The Electric and Magnetic Field Instrument Suite and Integrated Science (EMFISIS) on RBSP (2013, background): “Unfortunately, recent satellite observations (Chum et al. 2007; Breneman et al. 2009; Santolik et al. 2009; Haque et al. 2010) indicate a wide range of values for this key property, which adds uncertainty to modeling studies.”
- Radiation belt dynamics: The importance of wave‐particle interactions (2010, background): “Unfortunately, recent satellite observations [Chum et al., 2007; Breneman et al., 2009; Santolík et al., 2009; Haque et al., 2010] indicate a wide range of values for this key property, which adds uncertainty to modeling studies.”
- Earth's Van Allen Radiation Belts: From Discovery to the Van Allen Probes Era (2019, background): “…Burtis & Helliwell, 1969; Koons & Roeder, 1990; Tsurutani & Smith, 1974) and often exhibit coherent, discrete elements, such as rising or falling tones with subpacket structures (Burton & Holzer, 1974; Crabtree et al., 2017; Gao et al., 2014; Li et al., 2012; Santolík et al., 2009, 2003, 2014).”
- Modeling the evolution of chorus waves into plasmaspheric hiss (2011, background): “, 2003] to ring‐like [Santolik et al., 2009] and oblique [Lefeuvre and Helliwell, 1985; Hayakawa et al.”
- Fine structure of large‐amplitude chorus wave packets (2014, background): “However, linear cold plasma theory shows that significant effects can be expected only very close to the whistler mode resonance angle [e.g., Santolík et al., 2009].”
- 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].”