1·This magnetic storm has different physical processes at the middle low latitudes and the southern polar cusp region.
分析表明，南极极隙区与中低纬区磁暴形态差异很大。
2·But without a large prominence eruption, we will not have a magnetic storm here at Earth that drives the brilliant aurora.
但是，如果不发生大喷发，地球将不会受磁暴影响，也就不会产生明亮的极光。
3·The compression and rotation of the magnetic field serve as an efficient mechanism to cause a large geomagnetic storm.
激波对磁云内禀磁力线的压缩和旋转被证实是增强地磁效应的有效机制。
4·It is shown that the trapped region will be greatly disturbed during the magnetic storm, and the particle number will vary accordingly.
计算结果认为在磁扰期间捕获区将要发生变化。这个变化引起了捕获区内粒子数目的变化。
5·Therefore ground-based observations of the magnetic storm is the most basic understanding of the magnetosphere, the most effective means.
因此磁暴的地面观测是了解磁层的最基本、最有效的手段。
6·Some new methods, included satellite thermal IR anomaly, earthquake cloud, double magnetic storm time method, the abnormal superimposition of tide-generating force resonance and so on, are introduced.
地震预报，特别是短临预报一直是个世界性的科学难题。介绍了几种地震预报的新方法、新途径，包括：卫星热红外异常法、地震云法、磁暴二倍法、引潮力共振的异常叠加法等。
7·Environmental Magnetic measurements were carried out on all urban dust, topsoil and dust storm samples.
对尘土、不同深度的表土和沙尘暴样品开展了系统的环境磁学参数测量。