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Cluster Post Launch Support (Apr 2010-Dec2010)

Cluster Post Launch Support (Apr 2010-Dec2010)
集群启动后支持(2010 年 4 月至 2010 年 12 月)
批准号:
ST/I001042/1
负责人:
Andrew Fazakerley
金额:
$27.09万
依托单位:
依托单位国家:
英国
项目类别:
Research Grant
财政年份:
2010
资助国家:
英国
项目状态:
已结题
起止时间:
2010 至 --

项目摘要

项目成果

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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 raising science questions for the future NASA Magnetospheric Multi-scale Mission. 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 the end of 2010 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
DOI: 10.5194/angeo-29-2131-2011
发表时间: 2011
期刊: Annales Geophysicae
影响因子: 1.9
作者: [Beyene S]
通讯作者: Beyene S
Global reconnection topology as inferred from plasma observations inside Kelvin-Helmholtz vortices
从开尔文-亥姆霍兹涡旋内的等离子体观测推断出的全局重联拓扑
DOI: 10.5194/angeo-28-893-2010
发表时间: 2010
期刊: Annales Geophysicae
影响因子: 1.9
作者: [Bavassano Cattaneo M]
通讯作者: Bavassano Cattaneo M
DOI: 10.1029/2009ja014587
发表时间: 2010-05
期刊: Journal of Geophysical Research
影响因子: --
作者: [Y. Asano;I. Shinohara;A. Retinò;P. Daly;E. Kronberg;T. Takada;R. Nakamura;Y. Khotyaintsev;]
通讯作者: Y. Asano;I. Shinohara;A. Retinò;P. Daly;E. Kronberg;T. Takada;R. Nakamura;Y. Khotyaintsev;
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
9
    Cluster Post-Launch Support (Oct 2009 - Mar 2010)
    • 批准号:
      ST/H004130/1
    • 项目类别:
      Research Grant
    • 资助金额:
      $22.2万
    • 财政年份:
      2009
    • 负责人:
      Andrew Fazakerley
    • 依托单位:
    Cluster Post-Launch Support 2008-2010
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      ST/G008493/1
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    • 资助金额:
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    • 资助金额:
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      2007
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      22361048
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    • 批准号:
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    • 项目类别:
      面上项目
    • 资助金额:
      52万元
    • 批准年份:
      2022
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    AGB和post-AGB星的星周尘埃与实测红外色指数
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      10973004
    • 项目类别:
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    • 资助金额:
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      2009
    • 负责人:
      姜碧沩
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    Post-WIMP用户界面模型和支撑技术研究
    • 批准号:
      60503054
    • 项目类别:
      青年科学基金项目
    • 资助金额:
      23.0万元
    • 批准年份:
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    • 负责人:
      田丰
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