By Zhenpeng Su
This thesis specializes in the development and alertness of an electron radiation belt kinetic version together with a number of adiabatic and non-adiabatic methods. The terrestrial radiation belt was once came upon over 50 years in the past and has acquired a resurgence of curiosity in recent times. the most drivers of radiation belt examine are the basic technology questions surrounding its advanced and dramatic dynamics and especially its capability risks posed to space-borne structures. The institution of physics-based radiation belt types may be in a position to establish the contributions of assorted mechanisms, forecast the long run radiation belt evolution after which mitigate its hostile house climate effects.
Dr. Su is now an Professor works in division of Geophysics and Planetary Sciences, collage of technological know-how and expertise of China, Hefei, China.
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Extra info for A Global Kinetic Model for Electron Radiation Belt Formation and Evolution
The solid and dashed lines represent the simulations with and without cross diffusion can drive the electrons with the large pitch-angles toward the loss cone. Hence, the combination of hiss and EMIC waves would produce more effective precipitation loss of radiation belt electrons (Li et al. 2007; Su et al. 2011c). 4 Conclusions and Discussions 31 (a) (b) (c) (d) Fig. 4 Conclusions and Discussions We have developed an electron radiation belt local diffusion model based on the quasilinear theory.
1988; Thorne et al. 2005). 2. The magnetic perturbation D LML tends to dominant throughout the outer radiation belt, while the electric perturbations are dominant in the slot region and inner belt. Stronger electric perturbation can lead to the filling of slot region and extremely large electron flux near the Earth. 0) are shown in Fig. 3. 090 MeV (Thorne et al. 2007) are also plotted for comparison. The obtained stable configuration, inner and outer belts separated by slot region (2−3Re ), can be clearly distinguished, generally comparable with the previous observations (Thorne et al.
1029/ 2004JA010628 Li W, Shprits YY, Thorne RM (2007) Dynamic evolution of energetic outer zone electrons due to wave-particle interactions during storms. 1029/ 2007JA012368 Lyons LR (1974a) Electron diffusion driven by magnetospheric electrostatic waves. J Geophys Res 79:575–580. 1029/JA079i004p00575 Lyons LR (1974b) General relations for resonant particle diffusion in pitch angle and energy. J Plasma Phys 12:45. 1017/S0022377800024910 Lyons LR (1974c) Pitch angle and energy diffusion coefficients from resonant interactions with ion-cyclotron and whistler waves.
A Global Kinetic Model for Electron Radiation Belt Formation and Evolution by Zhenpeng Su