Rebuilding process of the outer radiation belt during the 3 November 1993 magnetic storm: NOAA and Exos‐D observations

By Yoshizumi Miyoshi, A. Morioka, H. Misawa, T. Obara, T. Nagai, Y. Kasahara. 2003

272 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/1878e0ff155fed25848a2fab086d9550b1e3e3b5

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In Astronomy and Astrophysics

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

In Molecular Biology

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

Citations in the corpus

• Nonlinear mechanisms of lower-band and upper-band VLF chorus emissions in the magnetosphere (2009, background): “…radiation belt electrons [Summers et al., 1998, 2002, 2004a,b, 2007a,b; Roth et al., 1999;47 Summers and Ma, 2000; Albert, 2000, 2002; Miyoshi et al., 2003; Horne et al., 2005;48 Omura et al., 2007; Katoh and Omura, 2004, 2007a; Summers and Omura, 2007; Furuya49 et al., 2008; Katoh…”
• Corotating solar wind streams and recurrent geomagnetic activity: A review (2006, background): “…chorus is typically detected primarily close to the magnetic equator during substorms [Tsurutani and Smith, 1974], the sensitive wide band receiver and multichannel analyzers [Kimura et al., 1990] detected chorus during a magnetic storm in the off-equatorial regions as well [Miyoshi et al., 2003].”
• Relativistic electron precipitation by EMIC waves from self‐consistent global simulations (2008, background): “These low-energy electrons may be subsequently accelerated (on time scales of hours to days) to relativistic energies either by ultralow-frequency (ULF) waves [Rostoker et al., 1998; Elkington et al., 2004] or higher-frequency (VLF) chorus waves [e.g., Summers et al., 1998; Miyoshi et al., 2003; H”
• Outward radial diffusion driven by losses at magnetopause (2006, background): “Brautigam and Albert [2000] and Miyoshi et al. [2003] performed radial diffusion simulations of individual storms with variable outer boundary conditions derived from geosynchronous satellite measurements.”
• Timescales for radiation belt electron acceleration and loss due to resonant wave‐particle interactions: 2. Evaluation for VLF chorus, ELF hiss, and electromagnetic ion cyclotron waves (2007, methodology): “, 1999], the quasi-linear diffusion formalism [Summers and Ma, 2000; Summers et al., 2002, 2004b; Miyoshi et al., 2003; Horne et al., 2005a, 2005b; Varotsou et al., 2005; Shprits et al., 2006a], and a self-consistent wave-particle simulation code [Katoh and Omura, 2004] confirm that electron acceler”
• Theory and simulation of the generation of whistler‐mode chorus (2008, unknown): “In particular, energy diffusion due to electron gyroresonance with chorus is a key mechanism for generating relativistic electrons in the region 3 Miyoshi et al., 2003; Katoh and Omura, 2004; Summers, 2005; Horne et al., ...”
• Radiation Belt Environment model: Application to space weather nowcasting (2008, background): “Several studies have shown an association between relativistic electron flux enhancements and prolonged periods of enhanced chorus amplitudes lasting for the order of several days [Meredith et al., 2002, 2003a; Miyoshi et al., 2003 ].”
• Modeling the propagation characteristics of chorus using CRRES suprathermal electron fluxes (2007, unknown): “…et al., 1998, 2004; Horne et al., 2003, 2005a, 2005b; Thorne et al., 2005a, 2005b; Spasojevic and Inan, 2005; Meredith et al., 2002a, 2002b, 2003b; Miyoshi et al., 2003; Lyons et al., 2005; Smith et al., 2004; Varotsou et al., 2005; Shprits et al., 2006] playing a dual role in both the…”
• Precipitation of radiation belt electrons by EMIC waves, observed from ground and space (2008, background): “Whistler mode waves are essential for both non-adiabatic acceleration of relativistic electrons and pitch angle scattering [e.g., Lyons and Thorne, 1973; Li et al., 2007], and recent studies have shown that acceleration caused by whistler mode waves is very important for the flux enhancements of rel”
• The dual role of ELF/VLF chorus waves in the acceleration and precipitation of radiation belt electrons (2007, background): “Similar association of acceleration periods with chorus have been observed from space (Meredith et al., 2002a, b; Miyoshi et al., 2003; Meredith et al., 2003b).”
• On the storm‐time evolution of relativistic electron phase space density in Earth's outer radiation belt (2013, background): “…PSD distributions in L* [e.g., Green and Kivelson, 2004; Chen et al., 2007; Turner et al., 2012b], local acceleration within the outer belt [e.g., Miyoshi et al., 2003; Chen et al., 2007; Shprits et al., 2007; Turner et al., 2010; Schiller et al., 2012], and Mu-dependent L* distributions of PSD…”
• High‐speed solar wind with southward interplanetary magnetic field causes relativistic electron flux enhancement of the outer radiation belt via enhanced condition of whistler waves (2013, unknown): “0094-8276/13/10.1002/grl.50916 GEOPHYSICAL RESEARCH LETTERS, VOL. 40, 4520–4525, doi:10.1002/grl.50916, 2013 [e.g., Meredith et al., 2001; Miyoshi et al., 2003].”
• Geospace exploration project ERG (2018, background): “During the internal acceleration process (red arrows), sub-relativistic electrons are accelerated to MeV energies by whistler mode waves inside the radiation belts (e.g., Summers et al. 1998; Miyoshi et al. 2003; Thorne 2010).”
• Relativistic turning acceleration of resonant electrons by coherent whistler mode waves in a dipole magnetic field (2007, background): “[2] Over the course of a geomagnetic storm, the flux of relativistic (>1 MeV) electrons in the outer radiation belt (3 Miyoshi et al. [2003] , Miyoshi and Kataoka [2005].”
• THEMIS analysis of observed equatorial electron distributions responsible for the chorus excitation (2010, background): “tions [Tsurutani and Smith, 1974; Meredith et al., 2001, 2003; Miyoshi et al., 2003] in association with enhanced fluxes of suprathermal electrons [Anderson and Maeda, 1977; Meredith et al.”
• Energization of relativistic electrons in the presence of ULF power and mev microbursts: Evidence for dual ULF and VLF acceleration (2003, background): “Also, some case studies have found that radial diffusion is unable to reproduce the observed behavior of the radiation belts during selected storms [Brautigam and Albert, 2000; Miyoshi et al., 2003].”