中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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CAS IR Grid
机构
国家空间科学中心 [4]
采集方式
OAI收割 [4]
内容类型
期刊论文 [4]
发表日期
2011 [1]
2008 [1]
2007 [1]
2003 [1]
学科主题
空间物理 [4]
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Kinematic Evolution of a Slow CME in Corona Viewed by STEREO-B on 8 October 2007
期刊论文
OAI收割
SOLAR PHYSICS, 2011, 卷号: 269, 期号: 2, 页码: 389-400
作者:
Shen, Chenglong
;
Wang, Yuming
;
Gui, Bin
;
Ye, Pinzhong
;
Wang, S.
收藏
  |  
浏览/下载:25/0
  |  
提交时间:2014/12/15
Coronal mass ejections
Kinematic evolution
Heliospheric magnetic field
Global structure and dynamics of large-scale fluctuations in the solar wind: Voyager 2 observations during 2005 and 2006
期刊论文
OAI收割
Journal of Geophysical Research-Space Physics, 2008, 卷号: 113, 期号: A2, 页码: A02104
Burlaga, L. F.
;
Ness, N. F.
;
Acuna, M. H.
;
Wang, Y. M.
;
Sheeley, N. R.
;
王赤
;
Richardson, J. D.
收藏
  |  
浏览/下载:36/0
  |  
提交时间:2014/04/30
merged interaction region
heliospheric magnetic-field
outer
heliosphere
pickup ions
interplanetary shocks
termination shock
cosmic-rays
95 au
speed
evolution
Three-dimensional MHD simulation of CMEs in three-dimensional background solar wind with the self-consistent structure on the source surface as input: Numerical simulation of the January 1997 Sun-Earth connection event
期刊论文
OAI收割
Journal of Geophysical Research-Space Physics, 2007, 卷号: 112, 期号: A6, 页码: A06109
Shen, F.
;
Feng, X.
;
Wu, S. T.
;
Xiang, C. Q.
收藏
  |  
浏览/下载:25/0
  |  
提交时间:2014/04/30
coronal mass ejections
interplanetary shock-waves
heliospheric
current sheet
space weather
magnetic-field
magnetohydrodynamic
simulation
scintillation observations
flux rope
1 au
model
Global distribution of coronal mass outputs and its relation to solar magnetic field structures
期刊论文
OAI收割
Journal of Geophysical Research-Space Physics, 2003, 卷号: 108, 期号: A6, 页码: 1238
Wei, F. S.
;
Feng, X. S.
;
Cai, H. C.
;
Zhou, Q. J.
收藏
  |  
浏览/下载:46/0
  |  
提交时间:2014/04/30
coronal mass output flux
solar magnetic field
current sheet
global
structure
heliospheric current sheet
interplanetary scintillation
observations
streamer structure
wind structure
energy-flow
evolution
speed
sun
origin
models