Evolution

A Global Kinetic Model for Electron Radiation Belt Formation by Zhenpeng Su

By Zhenpeng Su

This thesis makes a speciality of the development and alertness of an electron radiation belt kinetic version together with a number of adiabatic and non-adiabatic techniques. The terrestrial radiation belt used to be found over 50 years in the past and has obtained a resurgence of curiosity in recent times. the most drivers of radiation belt examine are the basic technological know-how questions surrounding its advanced and dramatic dynamics and especially its strength risks posed to space-borne structures. The institution of physics-based radiation belt types might be in a position to determine the contributions of varied mechanisms, forecast the long run radiation belt evolution after which mitigate its opposed house climate effects.

Dr. Su is now an Professor works in division of Geophysics and Planetary Sciences, collage of technology and expertise of China, Hefei, China.

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1007/s00585-999-0631-2 Russell CT, Holzer RE, Smith EJ (1969) OGO 3 observations of ELF noise in the magnetosphere. 1. Spatial extent and frequency of occurrence. J Geophys Res 74:755–777. 1029/JA074i003p00755 Santolík O, Gurnett DA, Pickett JS, Parrot M, Cornilleau-Wehrlin N (2003) Spatio-temporal structure of storm-time chorus. J Geophys Res 108:1278. 1029/2002JA009791 Santolík O, Gurnett DA, Pickett JS, Parrot M, Cornilleau-Wehrlin N (2004) A microscopic and nanoscopic view of storm-time chorus on 31 March 2001.

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The including of cross diffusion often yields numerical instability for the common finite difference methods (Albert 2004; Albert and Young 2005). We propose an efficient, stable, and easily-programming numerical scheme, named HFD, to fully solve this diffusion equation (Su et al. 2009c, 2011c; Xiao et al. 2009). This numerical scheme has been widely used by our research group (Su et al. 2009a, b, c, 2010a, b, c, 2011a, b, c; Xiao et al. 2009, 2010b, a, 2011) and other researchers (Fok et al. 2010; Thorne et al.

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