The Electron Radiation Belt

By Xinlin Li, M. Temerin. 2001

163 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/9883b5fdc6defe5d53a78e69da01cca5a806570e

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. R. Horne
3. Nigel P. Meredith
4. Binbin Ni
5. Y. Shprits
6. S. Glauert
7. Danny Summers
8. Jacob Bortnik

In Geophysics

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

Citations in the corpus

• Statistical analysis of relativistic electron energies for cyclotron resonance with EMIC waves observed on CRRES (2003, background): “…responsible for stormtime acceleration [e.g., Li et al. , 1997; Elkington et al. , 1999; Summers and Ma , 2000a, 2000b; Hudson et al. , 2001; Li and Temerin , 2001; Mathie and Mann , 2001; Meredith et al. , 2001, 2002a, 2002b, 2003; O’Brien et al. , 2001; Friedel et al. , 2002; Summers et…”
• Three-dimensional simulations of outer radiation belt electron dynamics including cross-diffusion terms (2010, background): “... of flux has been regarded as the result of cyclotron wave‐particle interactions [Horne and Thorne, 1998; Summers et al., 1998, 2004, 2007a, 2007b; Roth et al., 1999; Summers and Ma, 2000; Horne et al., 2003a, 2005; L. Li et al., 2005; Iles et al., 2006; Xiao et al., 2006, 2007b, 2009a; Su et al.”
• Calculation of pitch angle and energy diffusion coefficients with the PADIE code (2005, background): “Enhanced radial transport and acceleration and loss by wave-particle interactions are thought to contribute significantly to these flux variations (e.g., see the reviews by Li and Temerin [2001] , Friedel et al. [2002], and Horne [2002]).”
• Relativistic electron acceleration and precipitation during resonant interactions with whistler‐mode chorus (2003, background): “Increases in flux are due to acceleration processes inside the Earth’s magnetosphere [Li et al., 1997a], but there is considerable debate over which is the most important mechanism [Li and Temerin, 2001; Friedel et al., 2002; Horne, 2002].”
• Energetic outer zone electron loss timescalesduring low geomagnetic activity (2006, background): “proposed (see the reviews by Li and Temerin [2001] , Horne [2002], and Friedel et al. [2002]), recent experimental and modelling work suggests that the acceleration is caused by a combination of enhanced inward radial diffusion driven by ULF waves [e.g., Elkington et al., 1999; Liu et al., 1999; Hu”
• Dynamics of the Earth’s Particle Radiation Environment (2009, background): “It has been established that electron acceleration occurs inside the magnetosphere (Li et al. 1997) and several possible acceleration mechanisms have been proposed (see the reviews by Li and Temerin 2001; Friedel et al. 2002; Horne 2002).”
• Timescales for radiation belt electron acceleration and loss due to resonant wave-particle interactions: 1. Theory (2007, background): “A broad discussion of the issues of radiation belt electron transport, acceleration, and loss is provided collectively in the papers by Li and Temerin [2001] , Friedel et al. [2002], O’Brien et al. [2003], Green and Kivelson [2004], Green et al. [2005], and Thorne et al. [2005a].”
• Nonlinear interaction of outer zone electrons with VLF waves (2002, background): “[2] The dynamics of electrons in the outer radiation belts pose an outstanding problem of great current interest [Li and Temerin, 2001].”
• Timescale for radiation belt electron acceleration by whistler mode chorus waves (2005, background): “[3] Several theories have been suggested to account for the acceleration (see the reviews by Li and Temerin [2001] , Friedel et al. [2002], and Horne [2002]).”
• 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, background): “[3] Processes governing the transport, acceleration, and loss of radiation belt electrons are discussed by Li et al. [1997], Summers and Ma [2000], Li and Temerin [2001] , Friedel et al. [2002], O’Brien et al. [2003], Green and Kivelson [2004], Green et al. [2005], and Thorne et al. [2005a].”