Cluster Post-Launch Support 2008-2010
Cluster Post-Launch Support 2008-2010
批准号:
ST/G008493/1
负责人:
Andrew Fazakerley
金额:
$45.0万
依托单位国家:
英国
项目类别:
Research Grant
财政年份:
2009
资助国家:
英国
项目状态:
已结题
起止时间:
2009 至 --
中文摘要
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英文摘要
The Cluster Mission, for the first time, is exploring the magnetosphere with a fleet of four spacecraft orbiting in a group. The magnetosphere is the region of space around the Earth in which the Earth's magnetic field can be detected. It is the operating environment for many spacecraft that affect our quality of life, such as weather, television and communications satellites, as well as scientific spacecraft used to study the Earth, the Sun and solar system, and the cosmos. The magnetosphere is occasionally a dangerous environment for spacecraft, and understanding why this is so is one of the motivations for the Cluster project. The original 2 year mission was extended to allow Cluster to investigate a range of phenomena with different scale sizes, by varying the size of the Cluster tetrahedron from year to year. More recently, the Cluster Multi-Scale Mission has been under way, in which 3 of the spacecraft are separated by ~10,000 km. The distance between one of these and the fourth spacecraft has been varied from a tiny 40 km (in space plasma terms) up to 10,000 km. This work is laying the foundations for the proposed Cross-Scale mission (see www.cross-scale.org). Another exciting aspect of the Cluster Multi-scale Mission is that it will visit regions of the magnetosphere which were previously unexplored by Cluster, including the places where the solar wind first meets the magnetosphere, where aurorae are generated and where some magnetospheric substorms originate. In all of these places, Cluster's 4 well instrumented spacecraft, will provide new data to reveal the plasma physical processes at work, which in turn will help us understand how the magnetosphere works. A Plasma Electron And Current Experiment (PEACE) instrument can measure the three dimensional velocity distribution of electrons in a space plasma, for an energy range from a few electronvolts to about 30 kiloelectronvolts, every 4 seconds. A PEACE instrument is flying on each of the four Cluster II spacecraft, and consists of two sensor units and a data processing unit. All 8 sensors and 4 DPUs are still working well, after 8 years in space, despite regular passages through the earth's radiation belts. PEACE can tell us about the density and temperature of the electron plasma near the spacecraft, whether it is flowing and how fast, and whether electron beams from energetic sources elsewhere are passing the spacecraft, guided by the local magnetic field - giving PEACE a remote sensing capability. PEACE can tell us about the electrical currents being carried by the electrons, which is important as such currents transmit forces throughout the magnetosphere. The four PEACE instruments working together can tell us whether there are local flow shears (as in a river where the water flows faster nearer the middle) or even eddies and vortices in the electron plasma; whether there are waves in the plasma or on plasma boundaries, and can determine pressure gradients. This is a unique measurement capability for Cluster, as the counterpart plasma ion instruments do not work on all four spacecraft. It is providing glimpses of the way that explosive energy release processes such a magnetic reconnection work, which is very important as such processes are very active on the Sun and throughout the cosmos. Similarly, PEACE is helping to reveal how collisionless shocks work. Shocks are also phenomena that likely occur throughout the cosmos, and which are capable of energising electrons and ions to very large energies. This grant will allow us to continue operating the PEACE instruments until late 2009 and to do essential work on data handling, processing and curation, and maintaining up-to-date instrument calibrations. All this is needed to enable us to make scientifically useful data available to the research community. It will also help us to play our part in constructing and populating the Cluster Active Archive being created by the European Space Agency.
期刊论文(10)
专著(0)
科研奖励(0)
会议论文
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Radial propagation velocity of energetic particle injections according to measurements onboard the Cluster satellites
根据集群卫星上的测量,高能粒子注入的径向传播速度
DOI:
10.1134/s0010952509010031
发表时间:
2009
期刊:
Cosmic Research
影响因子:
0.6
作者:
[Apatenkov S]
通讯作者:
Apatenkov S
DOI:
10.1002/2016ja022541
发表时间:
2016-07-01
期刊:
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
影响因子:
2.8
作者:
[Allen, R. C., Zhang, J. -C., Jordanova, V. K.]
通讯作者:
Jordanova, V. K.
Deriving plasma densities in tenuous plasma regions, with the spacecraft potential under active control
在主动控制航天器潜力的情况下推导出稀薄等离子体区域中的等离子体密度
DOI:
10.1002/2015ja021472
发表时间:
2015
期刊:
Space Physics
影响因子:
--
作者:
[Andriopoulou M]
通讯作者:
Andriopoulou M
DOI:
10.1002/2014ja020691
发表时间:
2015-02-01
期刊:
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
影响因子:
2.8
作者:
[Alm, L., Li, B., Karlsson, T.]
通讯作者:
Karlsson, T.
DOI:
10.1002/jgra.50408
发表时间:
2013
期刊:
Space Physics
影响因子:
--
作者:
[Alm L]
通讯作者:
Alm L
共 7 条
Cluster Post Launch Support (Apr 2010-Dec2010)
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批准号:ST/I001042/1
-
项目类别:Research Grant
-
资助金额:$27.09万
-
财政年份:2010
-
负责人:Andrew Fazakerley
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依托单位:
Cluster Post-Launch Support (Oct 2009 - Mar 2010)
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批准号:ST/H004130/1
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项目类别:Research Grant
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资助金额:$22.2万
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财政年份:2009
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负责人:Andrew Fazakerley
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依托单位:
MSSL PRD Case for Support: Plasma Analysers for KuaFu
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批准号:PP/E006752/1
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项目类别:Research Grant
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资助金额:$8.17万
-
财政年份:2007
-
负责人:Andrew Fazakerley
-
依托单位:
国内基金
海外基金
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基于可见光环化反应的Post-Iboga类吲哚生物碱不对称集群合成
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批准号:22361048
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项目类别:地区科学基金项目
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资助金额:32万元
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批准年份:2023
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负责人:潘志强
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基于菌群-肠-脑轴研究TMAO通过POST1/SREBP2调节星形胶质细胞胆固醇代谢参与针刺减轻糖尿病认知功能障碍的机制
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批准号:--
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项目类别:面上项目
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资助金额:52万元
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批准年份:2022
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负责人:王强
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依托单位:
AGB和post-AGB星的星周尘埃与实测红外色指数
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批准号:10973004
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项目类别:面上项目
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资助金额:45.0万元
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批准年份:2009
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负责人:姜碧沩
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依托单位:
Post-WIMP用户界面模型和支撑技术研究
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批准号:60503054
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项目类别:青年科学基金项目
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资助金额:23.0万元
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批准年份:2005
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负责人:田丰
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依托单位: