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极光半球能量季节变化与太阳活动周期的关联
郑玲; 傅绥燕; 宗秋刚; Parks George; 王赤; 陈曦
Department空间科学部
Source Publication科学通报
2013
Volume58Issue:9Pages:853-853
ISSN0023-074X
Language中文
Keyword极光半球能量 季节变化 太阳活动周期
Abstract极光半球能量(auroral hemispheric power,HP)是指通过极光沉降粒子进入地球南北半球的总能量,其南北半球不对称性或者季节不对称性早已为人们所熟知,即冬季半球的HP与同期夏季半球的HP存在差异,但对于究竟冬季半球还是夏季半球获取更多极光能量尚有争议,且迄今还没有关于极光能量半球不对称性与太阳周期关联的报道.
Indexed ByCSCD
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Document Type期刊论文
Identifierhttp://ir.nssc.ac.cn/handle/122/5067
Collection空间科学部
Recommended Citation
GB/T 7714
郑玲,傅绥燕,宗秋刚,等. 极光半球能量季节变化与太阳活动周期的关联[J]. 科学通报,2013,58(9):853-853.
APA 郑玲,傅绥燕,宗秋刚,Parks George,王赤,&陈曦.(2013).极光半球能量季节变化与太阳活动周期的关联.科学通报,58(9),853-853.
MLA 郑玲,et al."极光半球能量季节变化与太阳活动周期的关联".科学通报 58.9(2013):853-853.
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