中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
首页 机构 成果 学者
  
  1. CAS IR Grid
  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
A New Method to Comprehensively Diagnose Shock Waves in the Solar Atmosphere Based on Simultaneous Spectroscopic and Imaging Observations

文献类型：期刊论文

作者Ruan, Wenzhi1,4; Yan, Limei2; He, Jiansen1; Zhang, Lei3; Wang, Linghua1; Wei, Yong2
刊名ASTROPHYSICAL JOURNAL
出版日期2018-06-20
卷号860期号:2
ISSN号0004-637X
关键词shock waves Sun: atmosphere Sun: oscillations
DOI10.3847/1538-4357/aac0f8
文献子类Article
英文摘要Shock waves are believed to play an important role in plasma heating. The shock-like temporal jumps in radiation intensity and Doppler shift have been identified in the solar atmosphere. However, a quantitative diagnosis of the shocks in the solar atmosphere is still lacking, seriously hindering the understanding of shock dissipative heating of the solar atmosphere. Here, we propose a new method to realize the goal of the shock quantitative diagnosis, based on Rankine-Hugoniot equations and taking the advantages of simultaneous imaging and spectroscopic observations from, e.g., IRIS (Interface Region Imaging Spectrograph). Because of this method, the key parameters of shock candidates can be derived, such as the bulk velocity and temperature of the plasma in the upstream and downstream, the propagation speed and direction. The method is applied to the shock candidates observed by IRIS, and the overall characteristics of the shocks are revealed quantitatively for the first time. This method is also tested with the help of forward modeling, i.e., virtual observations of simulated shocks. The parameters obtained from the method are consistent with the parameters of the shock formed in the model and are independent of the viewing direction. Therefore, the method we proposed here is applicable to the quantitative and comprehensive diagnosis of the observed shocks in the solar atmosphere.
WOS关键词TRANSITION REGION OSCILLATIONS ; SLOW MAGNETOACOUSTIC WAVES ; SUNSPOT OSCILLATIONS ; CORONAL LOOPS ; POLAR PLUMES ; WIND ; SIGNATURE
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000435374600013
资助机构NSFC(41574168 ; NSFC(41574168 ; National Young Talent Program of China ; National Young Talent Program of China ; National Postdoctoral Program for Innovative Talents(BX201600159) ; National Postdoctoral Program for Innovative Talents(BX201600159) ; China Postdoctral Science Foundation(2017M610978) ; China Postdoctral Science Foundation(2017M610978) ; 41474148 ; 41474148 ; 41421003 ; 41421003 ; 41704166 ; 41704166 ; 41525016 ; 41525016 ; 41474155 ; 41474155 ; 41661164034) ; 41661164034) ; NSFC(41574168 ; NSFC(41574168 ; National Young Talent Program of China ; National Young Talent Program of China ; National Postdoctoral Program for Innovative Talents(BX201600159) ; National Postdoctoral Program for Innovative Talents(BX201600159) ; China Postdoctral Science Foundation(2017M610978) ; China Postdoctral Science Foundation(2017M610978) ; 41474148 ; 41474148 ; 41421003 ; 41421003 ; 41704166 ; 41704166 ; 41525016 ; 41525016 ; 41474155 ; 41474155 ; 41661164034) ; 41661164034) ; NSFC(41574168 ; NSFC(41574168 ; National Young Talent Program of China ; National Young Talent Program of China ; National Postdoctoral Program for Innovative Talents(BX201600159) ; National Postdoctoral Program for Innovative Talents(BX201600159) ; China Postdoctral Science Foundation(2017M610978) ; China Postdoctral Science Foundation(2017M610978) ; 41474148 ; 41474148 ; 41421003 ; 41421003 ; 41704166 ; 41704166 ; 41525016 ; 41525016 ; 41474155 ; 41474155 ; 41661164034) ; 41661164034) ; NSFC(41574168 ; NSFC(41574168 ; National Young Talent Program of China ; National Young Talent Program of China ; National Postdoctoral Program for Innovative Talents(BX201600159) ; National Postdoctoral Program for Innovative Talents(BX201600159) ; China Postdoctral Science Foundation(2017M610978) ; China Postdoctral Science Foundation(2017M610978) ; 41474148 ; 41474148 ; 41421003 ; 41421003 ; 41704166 ; 41704166 ; 41525016 ; 41525016 ; 41474155 ; 41474155 ; 41661164034) ; 41661164034)
源URL[http://ir.iggcas.ac.cn/handle/132A11/88189]  
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Ruan, Wenzhi
作者单位1.Peking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R China
2.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing 100029, Peoples R China
3.Chinese Acad Sci, State Key Lab Space Weather, Beijing 100190, Peoples R China
4.Katholieke Univ Leuven, Dept Math, Ctr Math Plasma Astrophys, Celestijnenlaan 200B, B-3001 Leuven, Belgium
推荐引用方式
GB/T 7714		 Ruan, Wenzhi,Yan, Limei,He, Jiansen,et al. A New Method to Comprehensively Diagnose Shock Waves in the Solar Atmosphere Based on Simultaneous Spectroscopic and Imaging Observations[J]. ASTROPHYSICAL JOURNAL,2018,860(2).
APA Ruan, Wenzhi,Yan, Limei,He, Jiansen,Zhang, Lei,Wang, Linghua,&Wei, Yong.(2018).A New Method to Comprehensively Diagnose Shock Waves in the Solar Atmosphere Based on Simultaneous Spectroscopic and Imaging Observations.ASTROPHYSICAL JOURNAL,860(2).
MLA Ruan, Wenzhi,et al."A New Method to Comprehensively Diagnose Shock Waves in the Solar Atmosphere Based on Simultaneous Spectroscopic and Imaging Observations".ASTROPHYSICAL JOURNAL 860.2(2018).

入库方式： OAI收割

来源：地质与地球物理研究所

浏览0
下载0
收藏0
其他版本

除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。