Determining and understanding substorm energy loss and partitioning
Determining and understanding substorm energy loss and partitioning
批准号:
NE/L007495/1
负责人:
Jonathan Rae
金额:
$34.24万
依托单位国家:
英国
项目类别:
Research Grant
财政年份:
2014
资助国家:
英国
项目状态:
已结题
起止时间:
2014 至 --
中文摘要
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英文摘要
The substorm is a repeatable earthquake-like disturbance to near-Earth Space, which, apparently unpredictably, recurs after anything from 2 hours to a day or more and dumps typically one thousand million million Joules of energy into the upper atmosphere equivalent to ten Oklahoma tornados or the largest nuclear weapon in the US arsenal. The substorm's intermittency and variable size makes it arguably the greatest source of uncertainty in predicting the state of the upper atmosphere. Its most obvious effect is the aurora, which would be nice to know when its happening so that we could plan our Arctic holidays, but substorm prediction is also important for mitigating the effects of natural changes in the upper atmosphere on geostationary satellite communications and navigation, low-altitude satellite orbits and remote sensing, electricity power grids, and oil and mineral prospecting. Prediction is also the ultimate test for our scientific understanding. Progress requires measuring and analysing substorm variability in order to test and develop models based on maths and physics. We already know the statistics of substorm timing and have explained this with a simple mathematical model (that has also been used for understanding neuron firing in the brain!). However, knowing and understanding the variability of substorm size is much harder because it requires to measure simultaneously over large regions of the polar upper atmosphere and out into Space.In this project, we propose to attempt this by examining lots of substorms over more than a decade using spacecraft together with networks of magnetometers (sophisticated scientific compasses) and radars in both the Arctic and Antarctic. The resulting stats will be compared with what we already know from much more limited observations and with the predictions of new and existing substorm theories and models. The outcomes will be knowing things like how likely a really big substorm is that could mess things up, as well as models to explain why and hopefully when that might occur.
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Spatial Distribution and Semiannual Variation of Cold-Dense Plasma Sheet
冷密等离子体片的空间分布及半年变化
DOI:
10.1002/2017ja024565
发表时间:
2018
期刊:
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
影响因子:
2.8
作者:
[Bai S., Shi Q., Tian A., Nowada M., Degeling A.W., Zhou X.-Z., Zong Q.-G., Rae I.J., Fu S., Zhang H., Pu Z., Fazakerly A.N.]
通讯作者:
Fazakerly A.N.
DOI:
10.1038/s41550-017-0262-6
发表时间:
2017-11-01
期刊:
NATURE ASTRONOMY
影响因子:
14.1
作者:
[Dunn, W. R., Branduardi-Raymont, G., Coates, A. J.]
通讯作者:
Coates, A. J.
DOI:
10.1002/2015ja021888
发表时间:
2016-03
期刊:
Journal of geophysical research. Space physics
影响因子:
--
作者:
[Dunn WR, Branduardi-Raymont G, Elsner RF, Vogt MF, Lamy L, Ford PG, Coates AJ, Gladstone GR, Jackman CM, Nichols JD, Rae IJ, Varsani A, Kimura T, Hansen KC, Jasinski JM]
通讯作者:
Jasinski JM
DOI:
10.1029/2018sw002102
发表时间:
2019-04
期刊:
Space Weather
影响因子:
--
作者:
[S. Bentley;C. Watt;I. J. Rae;M. Owens;K. Murphy;M. Lockwood;J. K. Sandhu]
通讯作者:
S. Bentley;C. Watt;I. J. Rae;M. Owens;K. Murphy;M. Lockwood;J. K. Sandhu
DOI:
10.1029/2017ja025147
发表时间:
2018-06
期刊:
Journal of Geophysical Research: Space Physics
影响因子:
--
作者:
[J. Coxon;M. Freeman;C. Jackman;C. Forsyth;I. J. Rae;R. Fear]
通讯作者:
J. Coxon;M. Freeman;C. Jackman;C. Forsyth;I. J. Rae;R. Fear
共 8 条
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财政年份:2020
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负责人:Jonathan Rae
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依托单位:
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依托单位:
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