作者: W.A. Coles
DOI: 10.1016/B978-0-08-042049-3.50090-9
关键词: Interplanetary magnetic field 、 Electron density 、 Astrophysics 、 Amplitude 、 Scintillation 、 Interplanetary medium 、 Physics 、 Scattering 、 Solar wind 、 Interplanetary scintillation
摘要: ABSTRACT Observations of interplanetary scintillation show that the spatial spectrum electron density in inner solar wind follows a Kolmogorov power-law at large scales. However scales 10's to 100's km there is well-defined excess. Angular scattering observations this excess region be highly anisotropic, least inside 10 Rs. Here we explore effect Alfven waves on observations, relationship fluctuations, and ways estimating wave amplitudes.