How does the aurora heat the upper atmosphere?
How does the aurora heat the upper atmosphere?
批准号:
NE/S015167/1
负责人:
Daniel Whiter
金额:
$67.51万
依托单位国家:
英国
项目类别:
Fellowship
财政年份:
2019
资助国家:
英国
项目状态:
未结题
起止时间:
2019 至 --
中文摘要
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英文摘要
My research will study the aurora, a beautiful display caused by energetic particles from space hitting the Earth's atmosphere at about 40 million mph. The aurora typically deposits 50 GW of power into the atmosphere, comparable to the electricity consumption of the UK. This huge energy source has considerable influence on the temperature and composition of the upper atmosphere, particularly in polar regions. The aurora is therefore one of many ingredients needed for computer simulations of the whole atmosphere, which predict changes to Earth's climate and to concentrations of gases such as ozone.Intense currents flow within and around aurora, heating the atmosphere just as an electric current heats a resistor. This heating has dramatic effects on the upper atmosphere, but several fundamental aspects remain undetermined. Previously it has been very difficult to measure the temperature of the atmosphere at auroral heights; it is too high for weather balloons, but too low for spacecraft. However, I recently made the exciting discovery, through experiment and theory, that the ratio of brightnesses of two specific auroral colours depends on the temperature of the atmosphere; therefore by observing these wavelengths in the aurora we can calculate the temperature. My idea is to use extremely sensitive cameras equipped with colour filters to make maps of atmospheric temperature, just like a thermal imaging camera. These temperature maps can be combined with radar measurements of the upper atmosphere to estimate the electrical conductivity, which is an important property influencing the flow of electric current through near-Earth space and the atmosphere. A computer simulation will help me to understand how different types of aurora are produced, what electric currents they generate, and how the aurora affects the temperature and chemistry of the upper atmosphere.
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DOI:
10.1029/2019ja027611
发表时间:
2020-08
期刊:
Journal of Geophysical Research: Space Physics
影响因子:
--
作者:
[J. Reidy;J. Reidy;R. Fear;D. Whiter;B. Lanchester;A. Kavanagh;Daniel J. Price;J. Chadney;Yongliang Zhang;L. Paxton]
通讯作者:
J. Reidy;J. Reidy;R. Fear;D. Whiter;B. Lanchester;A. Kavanagh;Daniel J. Price;J. Chadney;Yongliang Zhang;L. Paxton
DOI:
10.1007/s11214-019-0629-3
发表时间:
2020-01
期刊:
Space Science Reviews
影响因子:
10.3
作者:
[Y. Nishimura;M. Lessard;Y. Katoh;Y. Miyoshi;E. Grono;N. Partamies;Nithin Sivadas;K. Hosokawa;M. Fukizawa;M. Samara;R. Michell;R. Kataoka;T. Sakanoi;D. Whiter;S. Oyama;Y. Ogawa;S. Kurita]
通讯作者:
Y. Nishimura;M. Lessard;Y. Katoh;Y. Miyoshi;E. Grono;N. Partamies;Nithin Sivadas;K. Hosokawa;M. Fukizawa;M. Samara;R. Michell;R. Kataoka;T. Sakanoi;D. Whiter;S. Oyama;Y. Ogawa;S. Kurita
DOI:
10.1029/2022ja030628
发表时间:
2023
期刊:
Space Physics
影响因子:
--
作者:
[Krcelic P]
通讯作者:
Krcelic P
DOI:
10.5194/angeo-41-115-2023
发表时间:
2023-03
期刊:
Annales Geophysicae
影响因子:
1.9
作者:
[A. Goertz;N. Partamies;D. Whiter;L. Baddeley]
通讯作者:
A. Goertz;N. Partamies;D. Whiter;L. Baddeley
Characteristics of fragmented aurora-like emissions (FAEs) observed on Svalbard
在斯瓦尔巴群岛观测到的碎片状极光发射(FAE)的特征
DOI:
10.5194/angeo-39-277-2021
发表时间:
2021
期刊:
Annales Geophysicae
影响因子:
1.9
作者:
[Dreyer J]
通讯作者:
Dreyer J
共 9 条
EISCAT_3D: Fine-scale structuring, scintillation, and electrodynamics (FINESSE)
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批准号:NE/W003007/1
-
项目类别:Research Grant
-
资助金额:$50.46万
-
财政年份:2022
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负责人:Daniel Whiter
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依托单位:
Variability of neutral temperature in the high-latitude upper atmosphere
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批准号:NE/N004051/1
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项目类别:Research Grant
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资助金额:$48.16万
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财政年份:2016
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负责人:Daniel Whiter
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依托单位:
国内基金
海外基金
衍射光学三维信息加密与隐藏的研究
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批准号:60907004
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项目类别:青年科学基金项目
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资助金额:22.0万元
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批准年份:2009
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负责人:史祎诗
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依托单位: