依托于南北极科学考察,我国科学家利用南极中山站和北极黄河站位于极隙区纬度并构成地磁共轭的得天独厚的地理位置,可直接监测太阳风粒子进入极区高层大气引起的天气学现象。目前考察站已经建立了包括光学、无线电等探测手段在内的综合观测系统,自1995年以来对极区极光、电离层和地磁开展了持续监测。研究发现,太阳不断向外太空喷射带电粒子,形成所谓的太阳风。太阳风到达地球,与地球磁 Relying on the scientific exploration of the North and South Pole, our scientists can directly monitor the weather phenomena caused by the entry of the solar wind particles into the upper atmosphere of the polar region, using the favorable geographical location at the pole gap latitude of the Antarctic Zhongshan Station and the Arctic Yellow River Station. At present, the observation station has established an integrated observation system including detection methods such as optical and radio. Since 1995, it has conducted continuous monitoring of polar aurora, ionosphere and geomagnetic. The study found that the sun constantly jetting charged particles into space, the formation of the so-called solar wind. The solar wind reaches the Earth, magnetically with Earth