By Zhenpeng Su
This thesis makes a speciality of the development and alertness of an electron radiation belt kinetic version together with quite a few adiabatic and non-adiabatic methods. The terrestrial radiation belt was once came across over 50 years in the past and has bought a resurgence of curiosity in recent times. the most drivers of radiation belt examine are the basic technology questions surrounding its complicated and dramatic dynamics and especially its strength risks posed to space-borne platforms. The institution of physics-based radiation belt versions can be capable of determine the contributions of assorted mechanisms, forecast the long run radiation belt evolution after which mitigate its adversarial area climate effects.
Dr. Su is now an Professor works in division of Geophysics and Planetary Sciences, collage of technology and know-how of China, Hefei, China.
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Additional resources for A Global Kinetic Model for Electron Radiation Belt Formation and Evolution
Plasma Phys Controlled Fusion 50(062):001. 1088/0741-3335/50/6/062001 Xiao F, Su Z, Zheng H, Wang S (2009) Modeling of outer radiation belt electrons by multidimensional diffusion process. J Geophys Res 114(A03):201. 1029/2008JA013580 Xiao F, Chen L, Su Z, Zheng H, Wang S (2010a) A parametric study on outer radiation belt electron evolution by superluminous R-X mode waves. J Geophys Res 115(A10):217. 1029/2010JA015374 Xiao F, Su Z, Zheng H, Wang S (2010b) Three-dimensional simulations of outer radiation belt electron dynamics including cross diffusion terms.
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.
45) is solved by the alternative direction implicit (ADI) method (Strang 1968). The whole numerical algorithm is named as the Hybrid Finite Difference Method (HFD) due to the combination of two different finite difference methods. In the quasilinear dynamic simulations of radiation belt, ring current and aurora, this HFD method has been widely used by our group (Su et al. 2009a, b, c, 2010a, b, c, 2011a, b, c; Xiao et al. 2009, 2010a, b, 2011) and other researchers (Fok et al. 2010; Thorne et al.
A Global Kinetic Model for Electron Radiation Belt Formation and Evolution by Zhenpeng Su