作者: P. H. Yoon , L. F. Ziebell , R. Gaelzer , R. P. Lin , L. Wang
DOI: 10.1007/S11214-012-9867-3
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摘要: Charged particle acceleration takes place ubiquitously in the Universe including near-Earth heliospheric environment. Typical situ spacecraft measurements made solar wind show that charged velocity distribution contains energetic components with quasi scale-free power-law dependence, f∼v−α, for high range. In this Review a theory of quiet-time solar-wind electrons contain suprathermal component is discussed, which these are taken to be dynamical equilibrium Langmuir turbulence. This includes an overview turbulence theory, as well discussion on asymptotic solution turbulence/suprathermal electron system. Theoretical predictions high-energy index then compared against recent observations superhalo by instruments onboard WIND and STEREO spacecraft. It shown theoretical prediction intermediate observed