NSSC OpenIR  > 空间科学部
Alternative TitlePrediction Storms and Model of Magnetic Substomis
沈超; 刘振兴; 北京8701信箱
Source Publication中国基础科学
Keyword磁暴 磁层亚暴 理论预报模式 预报
Other AbstractMagnetic storms and substorms,important pnocess-es in the evolution of the geomagnetosphere.It is an urgent task to accurately predict the occurrence and strength of the magnetic stomps and substorms in space physics and space weather.Based on the theoretical analysis on the physical mechanism of magnetospheric dynamics,we have established an equivalent circuit method to predict stoma and substorms.With the observed solar wind parameters at the L1 point as the input conditions, this physical mode can well predict the evolution of the substornis and storms with leading times of about 50-80 rains and 2-3 hrs re-spectively.This physical prediction model can satisfy the need to ensure the safety and protection of space activities to certain extent.
Funding Project中国科学院空间科学与应用研究中心
Document Type期刊论文
Corresponding Author北京8701信箱
Recommended Citation
GB/T 7714
沈超,刘振兴,北京8701信箱. 磁暴和亚暴的理论预报模式[J]. 中国基础科学,2000(5):8-13.
APA 沈超,刘振兴,&北京8701信箱.(2000).磁暴和亚暴的理论预报模式.中国基础科学(5),8-13.
MLA 沈超,et al."磁暴和亚暴的理论预报模式".中国基础科学 .5(2000):8-13.
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