Determining and understanding substorm energy loss and partitioning
Determining and understanding substorm energy loss and partitioning
批准号:
NE/L007177/1
负责人:
Caitriona Jackman
金额:
$21.27万
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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DOI:
10.1002/2015ja021343
发表时间:
2015-12
期刊:
Journal of Geophysical Research: Space Physics
影响因子:
--
作者:
[C. Forsyth;I. J. Rae;J. Coxon;M. Freeman;C. Jackman;Jesper Gjerloev;Jesper Gjerloev;A. Fazakerley]
通讯作者:
C. Forsyth;I. J. Rae;J. Coxon;M. Freeman;C. Jackman;Jesper Gjerloev;Jesper Gjerloev;A. Fazakerley
DOI:
10.1002/2014gl062400
发表时间:
2014-12-28
期刊:
GEOPHYSICAL RESEARCH LETTERS
影响因子:
5.2
作者:
[Forsyth, C., Watt, C. E. J., Rae, I. J., Fazakerley, A. N., Kalmoni, N. M. E., Freeman, M. P., Boakes, P. D., Nakamura, R., Dandouras, I., Kistler, L. M., Jackman, C. M., Coxon, J. C., Carr, C. M.]
通讯作者:
Carr, C. M.
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
DOI:
10.1002/2015ja022050
发表时间:
2016-05-01
期刊:
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
影响因子:
2.8
作者:
[Coxon, J. C., Milan, S. E., Korth, H.]
通讯作者:
Korth, H.
How Well Can We Estimate Pedersen Conductance From the THEMIS White-Light All-Sky Cameras?
我们如何通过 THEMIS 白光全天相机估算 Pedersen 电导?
DOI:
10.1029/2018ja026067
发表时间:
2019
期刊:
Space Physics
影响因子:
--
作者:
[Lam M]
通讯作者:
Lam M
共 8 条
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项目类别:Fellowship
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资助金额:$57.9万
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财政年份:2014
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负责人:Caitriona Jackman
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依托单位:
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