Tiefpreis
CHF124.00
Print on Demand - Exemplar wird für Sie besorgt.
This 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 an Professor works in Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei, China.
Constructs a global kinetic model for the electron radiation belt formation and evolution Identifies the contributions of various adiabatic and non-adiabatic processes to the radiation belt dynamics Nominated as an Excellent Doctoral Dissertation Award of Chinese Academy of Sciences Includes supplementary material: sn.pub/extras
Autorentext
Dr. Su is now an Associate Professor works in Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei, China.
Honors:
Excellent Doctoral Dissertation Award of Chinese Academy of Sciences
Special Prize of the President Scholarship of Chinese Academy of Sciences
Publication list:
Su, Z. P., Xiao, F. L., Zheng, H. N., and Wang, S., Radiation belt electron dynamics driven by adiabatic transport, radial diffusion, and wave-particle interactions, J. Geophys. Res., 116, A04205, 2011.
Inhalt
Background and Motivation.- Local Diffusion.- Radial Diffusion.- Adiabatic Transport.- Magnetospheric Convection.- Summary.