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dc.contributor.authorSu, Zhenpengen_US
dc.date.accessioned2017-07-10T03:41:39Z
dc.date.available2017-07-10T03:41:39Z
dc.date.issued2015en_US
dc.identifier.isbn978-3-662-46650-6en_US
dc.identifier.isbn978-3-662-46651-3en_US
dc.identifier.otherHPU5160259en_US
dc.identifier.urihttps://lib.hpu.edu.vn/handle/123456789/26132
dc.description.abstractThis 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.en_US
dc.format.extent113 p.en_US
dc.format.mimetypeapplication/pdfen_US
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.subjectElectron Radiation Belt Formationen_US
dc.subjectA Global Kinetic Modelen_US
dc.subjectEvolutionen_US
dc.titleA Global Kinetic Model for Electron Radiation Belt Formation and Evolutionen_US
dc.typeThesisen_US
dc.size15,251Kben_US
dc.departmentTechnologyen_US


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