LEADER 03889nam 22007335 450 001 9910299450003321 005 20200702083227.0 010 $a3-662-46651-1 024 7 $a10.1007/978-3-662-46651-3 035 $a(CKB)3710000000379738 035 $a(EBL)3108788 035 $a(SSID)ssj0001465528 035 $a(PQKBManifestationID)11755382 035 $a(PQKBTitleCode)TC0001465528 035 $a(PQKBWorkID)11477849 035 $a(PQKB)11136145 035 $a(DE-He213)978-3-662-46651-3 035 $a(MiAaPQ)EBC3108788 035 $a(PPN)184896460 035 $a(EXLCZ)993710000000379738 100 $a20150325d2015 u| 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 12$aA Global Kinetic Model for Electron Radiation Belt Formation and Evolution /$fby Zhenpeng Su 205 $a1st ed. 2015. 210 1$aBerlin, Heidelberg :$cSpringer Berlin Heidelberg :$cImprint: Springer,$d2015. 215 $a1 online resource (113 p.) 225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 300 $aDescription based upon print version of record. 311 $a3-662-46650-3 320 $aIncludes bibliographical references. 327 $aBackground and Motivation -- Local Diffusion -- Radial Diffusion -- Adiabatic Transport -- Magnetospheric Convection -- Summary. 330 $aThis thesis focuses on the construction and application of an electron radiation belt kinetic model including various adiabatic and non-adiabatic processes. The terrestrial radiation belt was discovered over 50 years ago and has received a resurgence of interest in recent years. The main drivers of radiation belt research are the fundamental science questions surrounding its complex and dramatic dynamics and particularly its potential hazards posed to space-borne systems. The establishment of physics-based radiation belt models will be able to identify the contributions of various mechanisms, forecast the future radiation belt evolution, and then mitigate its adverse space weather effects.    Dr. Su is now a Professor works in Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei, China. . 410 0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 606 $aGeophysics 606 $aSpace sciences 606 $aPlasma (Ionized gases) 606 $aPhysics 606 $aGeophysics/Geodesy$3https://scigraph.springernature.com/ontologies/product-market-codes/G18009 606 $aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)$3https://scigraph.springernature.com/ontologies/product-market-codes/P22030 606 $aPlasma Physics$3https://scigraph.springernature.com/ontologies/product-market-codes/P24040 606 $aNumerical and Computational Physics, Simulation$3https://scigraph.springernature.com/ontologies/product-market-codes/P19021 606 $aGeophysics and Environmental Physics$3https://scigraph.springernature.com/ontologies/product-market-codes/P32000 615 0$aGeophysics. 615 0$aSpace sciences. 615 0$aPlasma (Ionized gases) 615 0$aPhysics. 615 14$aGeophysics/Geodesy. 615 24$aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). 615 24$aPlasma Physics. 615 24$aNumerical and Computational Physics, Simulation. 615 24$aGeophysics and Environmental Physics. 676 $a538.766 700 $aSu$b Zhenpeng$4aut$4http://id.loc.gov/vocabulary/relators/aut$01063187 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910299450003321 996 $aA Global Kinetic Model for Electron Radiation Belt Formation and Evolution$92530882 997 $aUNINA