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  2. 地质与地球物理研究所
  3. 中国科学院地质与地球物理研究所
  4. 中国科学院地球与行星物理重点实验室
IpsDst of Dst Storms Applied to Ionosphere-Thermosphere Storms and Low-Latitude Aurora

文献类型：期刊论文

作者Balan, N.1,2; Zhang, Qing -He2; Shiokawa, K.5; Skoug, R.4; Xing, Zanyang2; Ram, S. Tulasi3; Otsuka, Y.5
刊名JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
出版日期2019-11-01
卷号124期号:11页码:9552-9565
ISSN号2169-9380
DOI10.1029/2019JA027080
英文摘要Conventionally, the minimum value of Dst (DstMin) and maximum values of Kp and AE (Kp(max) and AE(max)) representing the geomagnetic storm intensities have been used for investigating space weather in Earth's environment. The present paper uses the derived parameters (IpsDst, IpsKp, and IpsAE) giving the mean values of Dst, Kp, and AE during the main phase (MP) of Dst storms for investigating ionosphere-thermosphere storms and low-latitude (630 nm) aurora. The derived parameters (IpsDst, IpsKp, and IpsAE) representing the impulsive strength of geomagnetic storms seem to have more systematic dependence among themselves than among the intensities (DstMin, Kpmax, and AEmax). The ionosphere-thermosphere storms observed by the CHAMP (Challenging Minisatellite Payload) satellite and low-latitude auroras observed by optical imagers are much more intense during high impulsive storms than high intensity storms. In a statistical sense, over 175 positive ionospheric storms (Delta NmF2) observed in 1985-2005 and the intensity of 20 red auroras observed in 1989-2004 at midlatitudes correlate better with the impulsive parameters than the intensity parameters, with the best correlation being with IpsDst. The mechanism of the impulsive action (high-energy input over a short duration) leading to large IpsDst arises from the impact of fast solar storms (interplanetary coronal mass ejections) with large IMF Bz southward at their front (or shock). The impulsive action results in bright low-latitude auroras and strong ionosphere-thermosphere storms.
WOS关键词MAGNETIC STORM ; SPACE WEATHER ; ELECTRIC-FIELDS ; RING CURRENT ; SOLAR-WIND ; EQUATORIAL ; DISTURBANCE ; INTENSITY ; PHASE ; ST
资助项目National Key R&D Program of China[2018YFC1407303] ; National Key R&D Program of China[2018YFC1407304] ; National Natural Science Foundation of China[41604139] ; National Natural Science Foundation of China[41574138] ; National Natural Science Foundation of China[41774166] ; National Natural Science Foundation of China[41431072] ; National Natural Science Foundation of China[41831072] ; Chinese Meridian Project ; foundation of National Key Laboratory of Electromagnetic Environment[6142403180103] ; foundation of National Key Laboratory of Electromagnetic Environment[6142403180102] ; JSPS KAKENHI in Japan[15H05815] ; JSPS KAKENHI in Japan[16H06286] ; U.S. Department of Energy ; NASA-ACE program
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000505404700087
出版者AMER GEOPHYSICAL UNION
资助机构National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project ; foundation of National Key Laboratory of Electromagnetic Environment ; foundation of National Key Laboratory of Electromagnetic Environment ; foundation of National Key Laboratory of Electromagnetic Environment ; foundation of National Key Laboratory of Electromagnetic Environment ; JSPS KAKENHI in Japan ; JSPS KAKENHI in Japan ; JSPS KAKENHI in Japan ; JSPS KAKENHI in Japan ; U.S. Department of Energy ; U.S. Department of Energy ; U.S. Department of Energy ; U.S. Department of Energy ; NASA-ACE program ; NASA-ACE program ; NASA-ACE program ; NASA-ACE program ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project ; foundation of National Key Laboratory of Electromagnetic Environment ; foundation of National Key Laboratory of Electromagnetic Environment ; foundation of National Key Laboratory of Electromagnetic Environment ; foundation of National Key Laboratory of Electromagnetic Environment ; JSPS KAKENHI in Japan ; JSPS KAKENHI in Japan ; JSPS KAKENHI in Japan ; JSPS KAKENHI in Japan ; U.S. Department of Energy ; U.S. Department of Energy ; U.S. Department of Energy ; U.S. Department of Energy ; NASA-ACE program ; NASA-ACE program ; NASA-ACE program ; NASA-ACE program ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project ; foundation of National Key Laboratory of Electromagnetic Environment ; foundation of National Key Laboratory of Electromagnetic Environment ; foundation of National Key Laboratory of Electromagnetic Environment ; foundation of National Key Laboratory of Electromagnetic Environment ; JSPS KAKENHI in Japan ; JSPS KAKENHI in Japan ; JSPS KAKENHI in Japan ; JSPS KAKENHI in Japan ; U.S. Department of Energy ; U.S. Department of Energy ; U.S. Department of Energy ; U.S. Department of Energy ; NASA-ACE program ; NASA-ACE program ; NASA-ACE program ; NASA-ACE program ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project ; foundation of National Key Laboratory of Electromagnetic Environment ; foundation of National Key Laboratory of Electromagnetic Environment ; foundation of National Key Laboratory of Electromagnetic Environment ; foundation of National Key Laboratory of Electromagnetic Environment ; JSPS KAKENHI in Japan ; JSPS KAKENHI in Japan ; JSPS KAKENHI in Japan ; JSPS KAKENHI in Japan ; U.S. Department of Energy ; U.S. Department of Energy ; U.S. Department of Energy ; U.S. Department of Energy ; NASA-ACE program ; NASA-ACE program ; NASA-ACE program ; NASA-ACE program
源URL[http://ir.iggcas.ac.cn/handle/132A11/95906]  
专题地质与地球物理研究所_中国科学院地球与行星物理重点实验室
通讯作者Balan, N.
作者单位1.Chinese Acad Sci, Inst Geol & Geophys, Beijing, Peoples R China
2.Shandong Univ, Inst Space Sci, Weihai, Peoples R China
3.Indian Inst Geomagnetism, Navi Mumbai, India
4.Los Alamos Natl Lab, Los Alamos, NM USA
5.Nagoya Univ, Inst Space Earth Environm Res, Nagoya, Aichi, Japan
推荐引用方式
GB/T 7714		 Balan, N.,Zhang, Qing -He,Shiokawa, K.,et al. IpsDst of Dst Storms Applied to Ionosphere-Thermosphere Storms and Low-Latitude Aurora[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2019,124(11):9552-9565.
APA Balan, N..,Zhang, Qing -He.,Shiokawa, K..,Skoug, R..,Xing, Zanyang.,...&Otsuka, Y..(2019).IpsDst of Dst Storms Applied to Ionosphere-Thermosphere Storms and Low-Latitude Aurora.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,124(11),9552-9565.
MLA Balan, N.,et al."IpsDst of Dst Storms Applied to Ionosphere-Thermosphere Storms and Low-Latitude Aurora".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 124.11(2019):9552-9565.

入库方式： OAI收割

来源：地质与地球物理研究所

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