行星际闪烁(IPS)研究新进展  

Interplanetary Scintillation (IPS) Observations

作　　者：马振国[1] 张喜镇[2] 韩文焌[2] 

机构地区：[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

出　　处：《天文学进展》2000年第3期209-215,共7页Progress In Astronomy

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。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.

关 键 词：太阳 太阳风 行星际闪烁 观测 

分 类 号：P182.9[天文地球—天文学]