Global model of lower band and upper band chorus from multiple satellite observations

By Nigel P. Meredith, R. Horne, A. Sicard-Piet, D. Boscher, K. Yearby, Wen Li, R. Thorne. 2012

253 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/c1ec810921c904e71585ac66f26605fdddbcdeaf

How researchers see this paper

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In Astronomy and Astrophysics

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

In Geophysics

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

Citations in the corpus

• Particle Dynamics in the Earth's Radiation Belts: Review of Current Research and Open Questions (2020, background): “…polarized whistler mode waves that are observed in two distinct frequency bands outside the plasmasphere up to geostationary orbits and beyond (e.g., Allcock, 1957; Bunch et al., 2013; LeDocq et al., 1998; Meredith et al., 2012; Meredith, Horne, Li, et al., 2014; Tsurutani & Smith, 1974).”
• Radiation belt electron acceleration by chorus waves during the 17 March 2013 storm (2014, background): “The latitudinal extent (|λ|) of chorus waves varies in different MLT sectors based on the statistical results [Meredith et al., 2012; Agapitov et al., 2013].”
• Three‐dimensional electron radiation belt simulations using the BAS Radiation Belt Model with new diffusion models for chorus, plasmaspheric hiss, and lightning‐generated whistlers (2014, background): “Electrons trapped in the Earth’s radiation belts encounter several different types of electromagnetic waves as they drift around the Earth, including whistler mode chorus, plasmaspheric hiss, and LGW.”
• Electron losses from the radiation belts caused by EMIC waves (2014, background): “Chorus waves tend to be most significant outside the plasmapause on the dawnside during active conditions [Meredith et al., 2001, 2012; Li et al., 2011].”
• Earth's Van Allen Radiation Belts: From Discovery to the Van Allen Probes Era (2019, methodology): “Before the Van Allen Probes era, empirical chorus wave distributions based on satellite wave measurements (Agapitov et al., 2013, 2018; Li et al., 2011, 2009; Meredith et al., 2012; Meredith, Horne, et al., 2003) were used to calculate diffusion coefficients driven by chorus waves.”
• Evolution and slow decay of an unusual narrow ring of relativistic electrons near L ~ 3.2 following the September 2012 magnetic storm (2013, background): “both chorus emissions, which are generated in the low density region outside the plasmapause [Meredith et al., 2012], and hiss, which is confined inside the plasmapause [Meredith et al.”
• Statistics of whistler mode waves in the outer radiation belt: Cluster STAFF‐SA measurements (2013, methodology): “Occurrence rate is quite close to the observed by THEMIS spacecraft in the equatorial region [Cully et al., 2008; Li et al., 2011; Meredith et al., 2012].”
• Global morphology and spectral properties of EMIC waves derived from CRRES observations (2014, methodology): “For our chorus wave database [Meredith et al., 2012] we initially averaged the wave data as a function of L∗ and half orbit in steps of 0.1L∗.”
• 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): “We assume a typical chorus wave frequency spectrum and wave normal distributions based on statistical results [Meredith et al., 2012; Li et al., 2011, 2013].”
• Statistical properties of plasmaspheric hiss derived from Van Allen Probes data and their effects on radiation belt electron dynamics (2015, background): “…chorus waves typically observed in the plasmatrough region with frequencies between 0.1 and 0.8 fce, where fce is the electron cyclotron frequency [e.g., Burtis and Helliwell, 1969; Burton and Holzer, 1974; Tsurutani and Smith, 1974, 1977; Meredith et al., 2003, 2012; Li et al., 2009, 2011].”
• Energetic electron precipitation associated with pulsating aurora: EISCAT and Van Allen Probe observations (2015, methodology): “Furthermore, it is assumed that LBC propagates to the magnetic latitude of 20°, based on the statistical analysis [Meredith et al., 2012].”