行星际闪烁(IPS)研究新进展

马振国1,2 张喜镇2 韩文俊2

(1. 中国科学院空间科学与应用研究中心 北京 100080)

(2. 中国科学院国家天文观测中心 北京 100012)

摘   要

太阳风行星际闪烁(interplanetary scintillation,IPS)研究在太阳物理、日地空间物理和空 间天气学研究中具有重要科学意义。经过近30年重点研究太阳风后,从90年代初开始,IPS 研究在太阳风与日球观测的对比分析、行星际扰动与地磁活动预报、观测数据的层析分析三方面 都取得了新的进展。

Interplanetary Scintillation (IPS) Observations

Ma Zhenguo1,2 Zhang Xizhen2 Han Wenjun2

(1 Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, 100080)

(2 National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012)

Abstract

The study of the interplanetary scintillation (IPS) of the solar wind is of great scientific significance in the fields of the solar physics, solar-terrestrial physics, as well as the newly developed space meteorology. By focusing on the observations of the solar wind during 30 years, more new progress has been made in the following three aspects with IPS observations since 1990s: the comparative analysis between the solar wind and the inner heliosphere, the interplanetary disturbance and the geomagnetic prediction, and the heliospheric data-tomography.

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