Electron-neutral collisions induced by artificially produced VLF waves: Radiation belt remediation
Electron-neutral collisions induced by artificially produced VLF waves: Radiation belt remediation
批准号:
ST/I000801/1
负责人:
Michael Denton
金额:
$10.28万
依托单位:
依托单位国家:
英国
项目类别:
Research Grant
财政年份:
2011
资助国家:
英国
项目状态:
已结题
起止时间:
2011 至 --
中文摘要
粒子与波的相互作用是自然界(例如太阳日冕的波粒加热)和实验室(例如磁约束托卡马克内等离子体的波粒加热)中发生的普遍物理过程。高功率无线电发射机的发展意味着现在可以沿着磁通量管发射甚低频信号,目的是在近地空间人为地诱导这种波-粒子相互作用。这项提议概述了一种称为辐射带补救的方法,通过使用这种甚低频信号人为地刺激电子-中性碰撞,减少辐射带中的高能电子数量。辐射带内不断变化的高能电子流量对轨道硬件是危险的,例如商业通信卫星,以及许多飞越该地区的科学和军事卫星。如果成功,所提出的研究将具有重大的实际应用,以及回答紧迫的物理问题。成功将提供一种手段,有可能保护航天器和仪器免受:(A)自然产生的粒子通量升高(例如,由于太阳驱动的变化和现场粒子加速,已知这是造成偶尔的卫星故障的原因);或(B)人为行动造成的极高通量(例如,高空核爆大量增加粒子通量,肯定会损坏穿越辐射带的卫星)。据估计,仅对美国政府卫星的辐射带干扰每年造成的损失就超过1亿美元(2000年以前),1994至1997年间,价值约5亿美元的卫星保险索赔是这种干扰的直接或间接结果。目前,需要昂贵的屏蔽来缓解这种影响,尽管任何数量的屏蔽都不能提供100%的保护。随着社会对天基技术的依赖与日俱增,显然,破坏的可能性和相关成本是巨大的。通过更好地了解造成这种影响的实际原因,以及随后开发减轻这些影响的手段,可以大大降低这种成本。
英文摘要
The interaction of particles and waves is a universal physical process that occurs in nature (e.g. wave-particle heating of the solar corona) as well as in the laboratory (e.g. wave-particle heating of plasmas within magnetic-confinement tokamaks). The development of high-powered radio-transmitters has meant that it is now possible to transmit very low frequency (VLF) signals along magnetic flux tubes with the aim of inducing such wave-particle interactions artificially in near-Earth space. This proposal outlines a method - known as radiation belt remediation - to decrease the number of energetic electrons in the radiation belts by artificially stimulating electron-neutral collisions using such VLF signals. The constantly changing flux of energetic electrons within the radiation belts is dangerous to orbiting hardware such as commercial communication satellites, and numerous scientific and military satellites which fly through the region. If successful, the research proposed would have significant practical applications as well as answering pressing physics problems. Success would provide a means to potentially protect spacecraft and instrumentation from: (a) the elevated particle fluxes that occur naturally (e.g. due to solar-driven variations and in situ particle acceleration, which are known to cause occasional satellite failure) or, (b) the exceptionally high fluxes that can occur due to human actions (e.g. high-altitude nuclear detonations massively increase particle fluxes and would certainly damage satellites traversing the radiation belts). It is estimated radiation-belt disruptions to USA government satellites alone cost in excess of $100 million per year (pre-2000) and that between 1994 and 1997 around $500 million worth of satellite insurance claims were a direct or indirect result of such disruptions. At present, expensive shielding is required to mitigate this effect, although no amount of shielding can provide 100% protection. With an ever-increasing societal reliance on space-based technology, it is clear that the potential for disruption and the related cost is huge. Such costs may be significantly reduced by better understanding the physical cause of such effects and by subsequent development of means to mitigate them.
期刊论文(10)
专著(0)
科研奖励(0)
会议论文
登录
查看更多内容
Statistically measuring the amount of pitch angle scattering that energetic electrons undergo as they drift across the plasmaspheric drainage plume at geosynchronous orbit
统计测量高能电子在地球同步轨道上的等离子层排水羽流中漂移时所经历的俯仰角散射量
DOI:
10.1002/2013ja019310
发表时间:
2014
期刊:
Space Physics
影响因子:
--
作者:
[Borovsky J]
通讯作者:
Borovsky J
Case studies of the impact of high-speed solar wind streams on the electron radiation belt at geosynchronous orbit: Flux, magnetic field, and phase space density
高速太阳风流对地球同步轨道电子辐射带影响的案例研究:通量、磁场和相空间密度
DOI:
10.1002/2013ja018923
发表时间:
2013
期刊:
Space Physics
影响因子:
--
作者:
[Hartley D]
通讯作者:
Hartley D
DOI:
10.1002/jgra.50524
发表时间:
2013-09
期刊:
Journal of Geophysical Research: Space Physics
影响因子:
--
作者:
[J. Borovsky;M. Denton]
通讯作者:
J. Borovsky;M. Denton
DOI:
10.1002/jgra.50292
发表时间:
2013
期刊:
Space Physics
影响因子:
--
作者:
[Forster D]
通讯作者:
Forster D
Electron number density, temperature, and energy density at GEO and links to the solar wind: A simple predictive capability
GEO 的电子数密度、温度和能量密度以及与太阳风的联系:简单的预测能力
DOI:
10.1002/2014ja019779
发表时间:
2014
期刊:
Space Physics
影响因子:
--
作者:
[Hartley D]
通讯作者:
Hartley D
共 8 条
Collaborative Research: Energetic Particle Precipitation from the Magnetosphere and Effects on Ozone Dynamics in the Mesosphere and Stratosphere
-
批准号:2123279
-
项目类别:Standard Grant
-
资助金额:$53.4万
-
财政年份:2022
-
负责人:Michael Denton
-
依托单位:
Autonomous observations of energetic particle effects on the Antarctic atmosphere
-
批准号:NE/H014330/1
-
项目类别:Research Grant
-
资助金额:$3.17万
-
财政年份:2010
-
负责人:Michael Denton
-
依托单位:
Acceleration and loss processes at relativistic energies: Sources and sinks of radiation belt plasma.
-
批准号:ST/G002401/1
-
项目类别:Research Grant
-
资助金额:$36.1万
-
财政年份:2009
-
负责人:Michael Denton
-
依托单位:
国内基金
海外基金
双星中性原子探测图像在地磁暴期间的时序演化过程反演分析
-
批准号:40974100
-
项目类别:面上项目
-
资助金额:45.0万元
-
批准年份:2009
-
负责人:路立
-
依托单位: