In 1967, a new type of radio telescope intended for the study of interplanetary scintillation came into operation. 1967年,一种新型的打算用于研究行星闪烁的射电望远镜投入了工作。
Inversion of the Spectrum of Solar Wind Electron Density Fluctuations in Interplanetary Scintillation Observation 行星际闪烁(IPS)观测中太阳风电子密度起伏谱的反演
The results of recent 30 years study of solar wind using the method of radio wave scattering are reviewed, with emphasis on the interplanetary scintillation ( IPS ). 本文以行星际闪烁(IPS)为主,综述了通过电波传播的观测来研究太阳风的方法及近30年的观测结果。
Single Station Interplanetary Scintillation Measurement to Diagnose Solar Wind Velocity 行星际闪烁(IPS)(IPS)单站观测对太阳风速度的诊断
The Fresnel structure in interplanetary scintillation power spectrum and solar-wind velocity 行星际闪烁(IPS)功率谱的Fresnel现象与太阳风速度