PMO OpenIR
freja卫星观测到的低混杂尖峰和密度空穴的因果关系
王德育1; Holback B2; 黄光力1; Queau K Le2
1996
Source Publication紫金山天文台台刊
ISSN1000-3681
Volume15Issue:2Pages:120
Abstract用非线性参量共振解释极光能化区离子回旋波的频率通常集中在二分之一的质子回旋频率附近的原因。假定离子回旋波已经存在,则非线性参量共振将预期其峰值频率恰好等于二分之一的质子回旋频率。由于非线性效应使参量共振趋于饱和,并导致共振频率的漂移。
Language英语
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/30181
Collection中国科学院紫金山天文台
Affiliation1.中国科学院紫金山天文台
2.Centre d'etude des Enovironnements Terrestre et Planetaires
First Author Affilication中国科学院紫金山天文台
Recommended Citation
GB/T 7714
王德育,Holback B,黄光力,等. freja卫星观测到的低混杂尖峰和密度空穴的因果关系[J]. 紫金山天文台台刊,1996,15(2):120.
APA 王德育,Holback B,黄光力,&Queau K Le.(1996).freja卫星观测到的低混杂尖峰和密度空穴的因果关系.紫金山天文台台刊,15(2),120.
MLA 王德育,et al."freja卫星观测到的低混杂尖峰和密度空穴的因果关系".紫金山天文台台刊 15.2(1996):120.
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