Overview of the Solar Polar Orbit Telescope Project for Space Weather Mission
查看参考文献113篇
文摘
The Solar Polar ORbit Telescope (SPORT) project for space weather mission has been under intensive scientific and engineering background studies since it was incorporated into the Chinese Space Science Strategic Pioneer Project in 2011. SPORT is designed to carry a suite of remote-sensing and in-situ instruments to observe Coronal Mass Ejections (CMEs), energetic particles, solar high-latitude magnetism, and the fast solar wind from a polar orbit around the Sun. The first extended view of the polar regions of the Sun and the ecliptic enabled by SPORT will provide a unique opportunity to study CME propagation through the inner heliosphere, and the solar high-latitude magnetism giving rise to eruptions and the fast solar wind. Coordinated observations between SPORT and other spaceborne/ground-based facilities within the International Living With a Star (ILWS) framework can significantly enhance scientific output. SPORT is now competing for official selection and implementation during China's 13th Five-Year Plan period of 2016—2020.
来源
空间科学学报
,2016,36(3):245-266 【核心库】
DOI
10.11728/cjss2016.03.245
关键词
Space weather
;
Coronal mass ejection
;
Solar magnetism
;
Solar wind
;
Solar energetic particle
地址
1.
National Space Science Center, Chinese Academy of Sciences, Beijing, 100190
2.
Center for Space Weather Sciences, Shandong University at Weihai, Weihai, 264200
3.
Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun, 130033
4.
Beijing Institute of Spacecraft System Engineering, China Aerospace Science and Technology Corporation, Beijing, 100094
5.
Shanghai Institute of Satellite Engineering, China Aerospace Science and Technology Corporation, Shanghai, 200030
6.
National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012
7.
Xi'an Institute of Optics and Precision Mechanics, Chinese Academy of Sciences, Xi'an, 710119
8.
School of Earth and Space Sciences, University of Science and Technology of China, Hefei, 230026
9.
Nanjing Institute of Astronomical Optics and Technology, Chinese Academy of Sciences, Nanjing, 210042
语种
英文
文献类型
研究性论文
ISSN
0254-6124
基金
Supported by the Strategic Priority Research Program on Space Science of Chinese Academy of Sciences
;
the Specialized Research Fund for State Key Laboratory of China, the Chinese National Science Foundation
;
the CAS/SAFEA international Partnership Program for Creative Research Teams
文献收藏号
CSCD:5698362
参考文献 共
113
共6页
1.
National Science and Technology Council.
National Space Weather Program Strategic Plan,2010
CSCD被引
1
次
2.
National Science and Technology Council.
National Space Weather Strategy: Space Weather Operations, Research, and Mitigation (SWORM) Task Force,2015
CSCD被引
2
次
3.
Belcher J W. Large-amplitude Alfven waves in the interplanetary medium, 2.
J. Geophys. Res,1971,76:3534-3563
CSCD被引
16
次
4.
Matthaeus W H. Measurement of the rugged invariants of magnetohydrodynamic turbulence in the solar wind.
J. Geophys. Res,1982,87:6011-6028
CSCD被引
6
次
5.
Tu C Y. MHD structures, waves and turbulence in the solar wind: observations and theories.
Space Sci. Rev,1995,73:1-210
CSCD被引
14
次
6.
Li B. Propagation of non-Wentzel-Kramers-Brillouin alfven waves in a multi-component solar wind with differential ion flow.
Astrophys. J,2007,661:1222-1233
CSCD被引
2
次
7.
Forbes T G. CME theory and models.
Space Sci. Rev,2006,123:251-302
CSCD被引
18
次
8.
Gopalswamy N. Properties of interplanetary coronal mass ejections.
Space Sci. Rev,2006,124:145
CSCD被引
1
次
9.
Webb D F. Coronal mass ejections: observations.
Living Rev. Solar Phys,2012,9:3
CSCD被引
13
次
10.
Gosling J T. Geomagnetic activity associated with Earth passage of interplanetary shock disturbances and coronal mass ejections.
J. Geophys. Res,1991,96:7831-7839
CSCD被引
21
次
11.
Zhang J. Solar and interplanetary sources of major geomagnetic storms (Dst ≤ -100nT) during 1996-2005.
J. Geophys. Res,2007,112(A10):A10102
CSCD被引
12
次
12.
Burlaga L F. Compound streams, magnetic clouds, and major geomagnetic storms.
J. Geophys. Res,1987,92:5725-5734
CSCD被引
5
次
13.
Burlaga L F. Successive CMEs and complex ejecta.
J. Geophys. Res,2002,107:1266
CSCD被引
5
次
14.
Wang Y M. Multiple magnetic clouds: several examples during March-April 2001.
J. Geophys. Res,2003,108:1370
CSCD被引
13
次
15.
Xiong M. Magnetohydrodynamic simulation of the interaction between interplanetary strong shock and magnetic cloud and its consequent geoeffectiveness.
J. Geophys. Res,2006,111:A08105
CSCD被引
3
次
16.
Xiong M. Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness.
J. Geophys. Res,2007,112:A11103
CSCD被引
9
次
17.
Shen C. Super-elastic collision of large-scale magnetized plasmoids in the heliosphere.
Nat. Phys,2012,8:923
CSCD被引
11
次
18.
Liu Y. Observations of an extreme storm in interplanetary space caused by successive coronal mass ejections.
Nat. Comm,2014,5:3481
CSCD被引
1
次
19.
Liu Y. A comprehensive view of the 2006 December 13 CME: from the Sun to interplanetary space.
Astrophys. J,2008,689:563-571
CSCD被引
4
次
20.
Zhang M. The hydromagnetic nature of solar coronal mass ejections.
Ann. Rev. Astron. Astrophys,2005,43:103-137
CSCD被引
20
次