The Double Star mission

被引:106
作者
Liu, ZX
Escoubet, CP
Pu, Z
Laakso, H
Shi, JK
Shen, C
Hapgood, M
机构
[1] European Space Agcy, ESTEC, SCI SH, NL-2200 AG Noordwijk, Netherlands
[2] Chinese Acad Sci, CSSAR, Beijing 100080, Peoples R China
[3] Peking Univ, Dept Geophys, Beijing 100871, Peoples R China
[4] Rutherford Appleton Lab, Didcot OX11 0QX, Oxon, England
关键词
magnetospheric physics; magnetopause; cusp; arid boundary layers; magnetotail; general or miscellaneous;
D O I
10.5194/angeo-23-2707-2005
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Double Star Programme (DSP) was first proposed by China in March, 1997 at the Fragrant Hill Workshop on Space Science, Beijing, organized by the Chinese Academy of Science. It is the first mission in collaboration between China and ESA. The mission is made of two spacecraft to investigate the magnetospheric global processes and their response to the interplanetary disturbances in conjunction with the Cluster mission. The first spacecraft, TC-1 (Tan Ce means "Explorer"), was launched on 29 December 2003, and the second one, TC-2, on 25 July 2004 on board two Chinese Long March 2C rockets. TC-1 was injected in an equatorial orbit of 570 x 79 000 km altitude with a 28 degrees inclination and TC-2 in a polar orbit of 560 x 38 000 km altitude. The orbits have been designed to complement the Cluster mission by maximizing the time when both Cluster and Double Star are in the same scientific regions. The two missions allow simultaneous observations of the Earth magnetosphere from six points in space. To facilitate the comparison of data, half of the Double Star payload is made of spare or duplicates of the Cluster instruments; the other half is made of Chinese instruments. The science operations are coordinated by the Chinese DSP Scientific Operations Centre (DSOC) in Beijing and the European Payload Operations Service (EPOS) at RAL, UK. The spacecraft and ground segment operations are performed by the DSP Operations and Management Centre (DOMC) and DSOC in China, using three ground station, in Beijing, Shanghai and Villafranca.
引用
收藏
页码:2707 / 2712
页数:6
相关论文
共 9 条
[1]   EXTREME ENERGETIC PARTICLE DECREASES NEAR GEOSTATIONARY ORBIT - A MANIFESTATION OF CURRENT DIVERSION WITHIN THE INNER PLASMA SHEET [J].
BAKER, DN ;
MCPHERRON, RL .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1990, 95 (A5) :6591-6599
[2]   The Double Star magnetic field investigation: instrument design, performance and highlights of the first year's observations [J].
Carr, C ;
Brown, P ;
Zhang, TL ;
Gloag, J ;
Horbury, T ;
Lucek, E ;
Magnes, W ;
O'Brien, H ;
Oddy, T ;
Auster, U ;
Austin, P ;
Aydogar, O ;
Balogh, A ;
Baumjohann, W ;
Beek, T ;
Eichelberger, H ;
Fornacon, KH ;
Georgescu, E ;
Glassmeier, KH ;
Ludlam, M ;
Nakamura, R ;
Richter, I .
ANNALES GEOPHYSICAE, 2005, 23 (08) :2713-2732
[3]   The STAFF-DWP wave instrument on the DSP equatorial spacecraft:: description and first results [J].
Cornilieau-Wehrlin, N ;
Alleyne, HS ;
Yearby, KH ;
de Vaux, BD ;
Meyer, A ;
Santolík, O ;
Parrot, M ;
Belmont, G ;
Rezeau, L ;
Le Contel, O ;
Roux, A ;
Attié, D ;
Robert, P ;
Bouzid, V ;
Herment, D ;
Cao, J .
ANNALES GEOPHYSICAE, 2005, 23 (08) :2785-2801
[4]   Coordinated Cluster/Double Star observations of dayside reconnection signatures [J].
Dunlop, MW ;
Taylor, MGGT ;
Davies, JA ;
Owen, CJ ;
Pitout, F ;
Fazakerley, AN ;
Pu, Z ;
Laakso, H ;
Bogdanova, YV ;
Zong, QG ;
Shen, C ;
Nykyri, K ;
Lavraud, B ;
Milan, SE ;
Phan, TD ;
Rème, H ;
Escoubet, CP ;
Carr, CM ;
Cargill, P ;
Lockwood, M ;
Sonnerup, B .
ANNALES GEOPHYSICAE, 2005, 23 (08) :2867-2875
[5]   The Cluster mission - Introduction [J].
Escoubet, CP ;
Fehringer, M ;
Goldstein, M .
ANNALES GEOPHYSICAE, 2001, 19 (10-12) :1197-1200
[6]  
Escoubet CP, 1997, SPACE SCI REV, V79, P1
[7]  
LIU Q, 1998, PRELIMINARY STUDY CO
[8]  
Lyons LR, 2000, ESA SPEC PUBL, V443, P255
[9]   Double Star project - master science operations plan [J].
Shen, C ;
Liu, Z .
ANNALES GEOPHYSICAE, 2005, 23 (08) :2851-2859