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太阳风及日冕物质抛射(CME)是地球空间环境扰动的主要驱动源,监测和研究太阳风对研究日地物理和进行日地空间环境预报具有重要意义.地基行星际闪烁观测为监测和研究太阳风及行星际空间提供了经济有效的手段.同时,行星际闪烁观测为研究激波、CME等现象的传播路径提供了有效途径,具有重大的科研和应用价值.我国行星际闪烁观测研究开始较晚,始于20世纪90年代.本文对我国行星际闪烁观测研究概况进行综述.
Solar wind and CME are the main driving forces for the disturbance of the Earth’s space environment. Monitoring and studying the solar wind is of great significance for the study of day-space physics and the prediction of the space environment on the earth’s surface. Interstellar space provides a cost-effective means.At the same time, intergalactic flicker observation provides an effective way to study the propagation path of shock wave, CME and other phenomena, and has great scientific value and application value.Research on intergalactic flicker observation started later in our country, In the 1990s, this paper summarized the research overview of intergalactic flicker observation in our country.