solar disturbance

We propose that the future forecasting of the physical conditions that the violent solar disturbance causes at the earth by propagating in solar wind depends heavily on the numerical method.

未来预测太阳剧烈扰动所造成的行星际风暴到达地球空间的状态势必借助于数值方法。

Its low amplitude makes it less important as a source of disturbance in magnetic prospecting than the solar component.

作为磁法勘探中的干扰源，它的幅度很小，所以远不及太阳日变分量那么重要。

Normal and quick run ( H. D.) records of the earth's magnetic field were made at Ruili, Yunnan Province during Feb. 16, 1980, total solar eclipse. Daily variation, small disturbance and magnetic pulsation were analysed.

1980年2月16日日全食期间，在云南瑞丽进行了地磁场的正常与快速两种记录，分析了地磁日变化、小扰动和地磁脉动的变化。

The solar activity, interplanetary disturbance and ground-based magnetic record during the three 2003 giant storms are investigated in this paper.

分析了引起2003年10～11月发生的3个特大磁暴的太阳活动、行星际扰动以及中国东部地磁台链记录到的地面磁场变化。

The second is to investigate the trigger mechanisms of magnetic storm, magnetospheric substorm, and magnetospheric particle storm, as well as the responses of magnetospheric space storm to the solar activities and interplanetary disturbance.

研究磁层亚暴、磁暴和磁层粒子暴的触发机制及磁层空间暴对太阳活动和行星际扰动的响应过程；

The Analysis of Antenna Noise Temperature During Solar Radiating Disturbance

日凌时天线噪声温度分析

Whereas in the vicinity of solar equator, propagating disturbance is regarded as fast mode wave, and a standing disturbance is found to be located near the source region.

而在赤道附近，传播扰动是快模磁声波，在源区附近还存在一非传播的扰动。

A new model of dealing with solar radiating disturbance is put forward and a systematic explanation to the antenna noise temperature analysis in case of solar radiating disturbance is made.

在提出日凌干扰处理新模型的基础上，根据太阳视面与天线主瓣半功率点截面的相对运动关系，系统阐述了日凌时天线噪声温度的分析方法。