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How Do Ultra-Low Frequency Waves Access the Inner Magnetosphere During Geomagnetic Storms?
Rae I.J.; Murphy K.R.; Watt C.E.J.; Sandhu J.K.; Georgiou M.; Degeling A.W.; Forsyth C.; Bentley S.N.; 等 更多
刊名Geophysical Research Letters
2019
卷号46期号:19页码:10699-10709
关键词radiation belt storm time ULF waves wave penetration
DOI10.1029/2019GL082395
URL标识查看原文
公开日期[db:dc_date_available]
内容类型期刊论文
URI标识http://www.corc.org.cn/handle/1471x/4549179
专题山东大学
作者单位1.Mullard Space Science Lab, UCL, Holmbury St Mary, United Kingdom
2.Department of Astronomy, University of Maryland, College Pa
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GB/T 7714
Rae I.J.,Murphy K.R.,Watt C.E.J.,et al. How Do Ultra-Low Frequency Waves Access the Inner Magnetosphere During Geomagnetic Storms?[J]. Geophysical Research Letters,2019,46(19):10699-10709.
APA Rae I.J..,Murphy K.R..,Watt C.E.J..,Sandhu J.K..,Georgiou M..,...&等 更多.(2019).How Do Ultra-Low Frequency Waves Access the Inner Magnetosphere During Geomagnetic Storms?.Geophysical Research Letters,46(19),10699-10709.
MLA Rae I.J.,et al."How Do Ultra-Low Frequency Waves Access the Inner Magnetosphere During Geomagnetic Storms?".Geophysical Research Letters 46.19(2019):10699-10709.
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