By Zhenpeng Su
This thesis makes a speciality of the development and alertness of an electron radiation belt kinetic version together with numerous adiabatic and non-adiabatic tactics. The terrestrial radiation belt used to be found 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 technological know-how questions surrounding its advanced and dramatic dynamics and especially its capability dangers posed to space-borne platforms. The institution of physics-based radiation belt types can be capable of establish the contributions of varied mechanisms, forecast the long run radiation belt evolution after which mitigate its opposed 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
Geophys Res Lett 31(L02):801. 1029/2003GL018757 Schulz M, Lanzerotti LJ (1974) Particle diffusion in the radiation belts, in physics and chemistry in space, vol 7. Springer, New York Shprits YY, Thorne RM, Horne RB, Glauert SA, Cartwright M, Russell CT, Baker DN, Kanekal SG (2006) Acceleration mechanism responsible for the formation of the new radiation belt during the 2003 halloween solar storm. Geophys Res Lett 33(L05):104. 1029/2005GL024256 Shprits YY, Elkington SR, Meredith NP, Subbotin DA (2008) Review of modeling of losses and sources of relativistic electrons in the outer radiation belt I: radial transport.
2009a). Based on previous works (Li et al. 2007; Summers et al. 2007b), we concentrate here on the parallelpropagating He+ band EMIC waves. The background ion composition is assumed to be 70 %H+ + 20 %He+ + 10 %O+ . 70 o+ . For such parallel-propagating L-mode waves, only the n = 1 order cyclotron resonance can occur (Summers 2005). The obtained diffusion rate distributions and profiles are plotted in Figs. 10. The modeled EMIC waves can only resonate with the high energy electrons (Summers 2005; Summers et al.
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. J Geophys Res 115(A05):216. 1029/ 2009JA014541 Xiao F, Chen L, He Y, Su Z, Zheng H (2011) Modeling of precipitation loss of ring current protons by electromagnetic ion cyclotron waves. J Atmos Sol Terr Phys 73:106–111. jastp. 007 Yoon PH (2011) Large-amplitude whistler waves and electron acceleration. Geophys Res Lett 381(L12):105.