行星际闪烁

关于利用行星际闪烁（IPS）观测进行地球磁暴急始预报的初步探讨

Preliminary results of predicting geomagnetic SSC by using IPS observations

根据行星际闪烁观测研究耀班一激波前后太阳风电子密度功率谱的变化

Study of variation the change in the electron density power spectra of solar wind before and after a Flare-shock using observed IPS data

行星际闪烁功率谱的Fresnel现象与太阳风速度

The Fresnel structure in interplanetary scintillation power spectrum and solar-wind velocity

行星际闪烁（IPS）单站观测对太阳风速度的诊断

Single Station Interplanetary Scintillation Measurement to Diagnose Solar Wind Velocity

行星际闪烁（IPS）观测中的几个问题

Some Aspects in Interplanetary Scintillation Observation

本文分析了第1733&1742Carrington周的太阳耀斑、行星际闪烁（IPS）、太阳风及K-日冕资料，对二维太阳风速度结构进行了综合研究。

The two-dimensional structure of solar wind speed with Carrington latitudes and longitudes is studied based on the analyses of the observations of flares , interplanetary scintillations .

行星际闪烁观测中太阳风电子密度起伏谱的反演

Inversion of the Spectrum of Solar Wind Electron Density Fluctuations in Interplanetary Scintillation Observation

本文在弱闪烁条件下，利用广泛适用于星际闪烁、行星际闪烁和电离层闪烁的薄相屏理论，以行星际闪烁为算例，对薄相屏闪烁进行了数值分析。

Under weak scintillation condition , computational analysis of interplanetary scintillations is given on the basis of phase-screen theory .

根据单站行星际闪烁的观测资料讨论耀斑激波前后的太阳风速度的变化

Discussion about the Change of the Solar Wind Velocity before and after the Flare-shock from Single Station IPS Data

本文以行星际闪烁为主，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。

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 ) .

太阳活动高年期间（19781981）耀斑-行星际激波传播的三维平均特性日本行星际闪烁（IPS）观测的初步分析

Three Dimensional Propagation Characteristics of the Flare-Associated Interplanetary Shock Wave During 1978-1981 INTERPLANETARY INTERMEDIATE SHOCK