Auroral Radio Emissions: A Window Into Electron Acceleration Processes
极光无线电发射:了解电子加速过程的窗口
基本信息
- 批准号:1915058
- 负责人:
- 金额:$ 19.9万
- 依托单位:
- 依托单位国家:美国
- 项目类别:Standard Grant
- 财政年份:2019
- 资助国家:美国
- 起止时间:2019-05-15 至 2025-04-30
- 项目状态:未结题
- 来源:
- 关键词:
项目摘要
The Northern Lights or aurorae result when energetic particles interact with the atmosphere ? producing a colorful sight in the night sky. The Arctic region near the North Pole is a prime location for viewing aurorae. This project is a follow-on to an NSF funded program that deployed and calibrated a receiver array in Toolik Lake, Alaska. This instrumentation will be used to view the aurorae and make new discoveries about how they are created. Graduate and undergraduate students will be trained and the scientific datasets will be shared with the public.A significant manifestation of high-latitude electromagnetic energy and particle flows is the terrestrial aurora which involves many acceleration processes affecting electrons and ions. These processes occur in both the magnetosphere and the ionosphere and are a key component of magnetosphere-ionosphere (M-I) coupling. Radio emissions from the accelerated auroral electron beams, with their complicated temporal and spatial variations, provide a window into the accelerated electron distributions and the processes that produce them. Auroral Medium Frequency Burst (MFB) emissions are especially promising in this regard because they are associated with substorm expansion arcs and exhibit structure on a range of time scales overlapping with those of Alfvenically accelerated suprathermal electron bursts and other phenomena such as flickering aurora. MFB is, however, relatively poorly understood: its source altitudes is not known, and although a mechanism has been proposed that suggests a connection to Alfvenic aurora, it has not been conclusively confirmed by observations. The proposed experiments, which will answer these and other outstanding questions about MFB and auroral radio emissions, are critical steps toward using MFB and its time and frequency structure as a diagnostic of auroral acceleration and nonlinear wave processes, to answer key questions about the temporal and spatial dynamics of these processes in the ionospheric context as well as their relation to larger dynamical processes such as storms and substorms.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.
当能量颗粒与大气相互作用时,北极光或极光会产生?在夜空中产生丰富多彩的景象。北极附近的北极地区是观看Aurorae的主要位置。该项目是NSF资助的计划的后续项目,该计划在阿拉斯加的Toolik Lake部署和校准了接收器阵列。该仪器将用于查看Aurorae,并就其创建方式进行新发现。将培训毕业生和本科生,并将与公众共享科学数据集。高纬度电磁能和粒子流的显着表现是地面极光,它涉及许多影响电子和离子的加速过程。这些过程都发生在磁层和电离层中,并且是磁层层(M-I)耦合的关键组成部分。来自加速的极光电子梁的无线电排放及其复杂的时间和空间变化为加速电子分布及其产生它们的过程提供了一个窗口。在这方面,极光中频率爆发(MFB)的排放尤其有希望,因为它们与近时间尺度上的近代膨胀弧和展示结构相关,并与Alfgenther上加速的超颗粒上电子爆发和其他现象(例如闪烁Aurora)重叠。但是,MFB的理解相对较少:尚不清楚其源高度,尽管提出了一种机制,提出了与Alfgenic Aurora有联系的机制,但尚未通过观察结果确认它。提出的实验将回答有关MFB和Auroral无线电排放的这些和其他杰出问题,是使用MFB及其时间和频率结构作为极光加速度和非线性波过程的关键步骤,以回答有关时间和时间和时间的关键问题这些过程在电离层环境中的空间动态及其与更大的动态过程(例如风暴和实体)的关系。该奖项反映了NSF的法定任务,并被认为是值得通过基金会的智力优点和更广泛的影响来通过评估来支持的。
项目成果
期刊论文数量(4)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)
A Statistical Study of Auroral Medium Frequency Bursts and Anomalous Incoherent Scatter Radar Echoes
极光中频爆发和异常非相干散射雷达回波的统计研究
- DOI:10.1029/2021rs007353
- 发表时间:2022
- 期刊:
- 影响因子:1.6
- 作者:Hudson, Emily;LaBelle, James;Reimer, Ashton;Akbari, Hassanali
- 通讯作者:Akbari, Hassanali
Langmuir Turbulence in the Auroral Ionosphere: Origins and Effects
极光电离层中的朗缪尔湍流:起源和影响
- DOI:10.3389/fspas.2020.617792
- 发表时间:2021
- 期刊:
- 影响因子:3
- 作者:Akbari, Hassanali;LaBelle, James W.;Newman, David L.
- 通讯作者:Newman, David L.
Estimating Polar Cap Density and Medium‐Frequency Burst Source Heights Using 2 f ce Roar Radio Emissions
使用 2 f ce 咆哮无线电发射估算极盖密度和中频爆发源高度
- DOI:10.1029/2020ja028166
- 发表时间:2020
- 期刊:
- 影响因子:0
- 作者:Burnett, Adam C.;LaBelle, James
- 通讯作者:LaBelle, James
Properties of the Stimulated Electromagnetic Emissions During the Inclined High‐Frequency Pumping of the Ionosphere Near the Fourth Electron Gyroharmonic at the High‐Frequency Active Auroral Research Program Facility
高频主动极光研究计划设施第四电子陀螺谐波附近电离层倾斜高频泵浦过程中受激电磁发射的特性
- DOI:10.1029/2019gl082890
- 发表时间:2019
- 期刊:
- 影响因子:5.2
- 作者:Shindin, A. V.;Grach, S. M.;Sergeev, E. N.;Smolina, V. P.;Pogorelko, N. A.;Bernhardt, P. A.;Briczinski, S. J.;Broughton, M.;LaBelle, J.;McCarrick, M. J.
- 通讯作者:McCarrick, M. J.
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James LaBelle其他文献
Perceptual structure of the desired functionality of internet-based health information systems
基于互联网的健康信息系统所需功能的感知结构
- DOI:
10.1007/s10729-006-7663-x - 发表时间:
2006 - 期刊:
- 影响因子:3.6
- 作者:
Imran S. Currim;V. Gurbaxani;James LaBelle;Jooseop Lim - 通讯作者:
Jooseop Lim
James LaBelle的其他文献
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{{ truncateString('James LaBelle', 18)}}的其他基金
First Conjugate-Station Studies and Continued Satellite-Conjunction Studies of LF/MF/HF Auroral Radio Emissions at South Pole
南极 LF/MF/HF 极光无线电发射的首次共轭站研究和持续卫星联合研究
- 批准号:
2205753 - 财政年份:2022
- 资助金额:
$ 19.9万 - 项目类别:
Standard Grant
Auroral Kilometric Radiation, Substorms, and Related Phenomena: Satellite Conjunction and Conjugate Studies at South Pole
极光千米辐射、亚暴和相关现象:南极的卫星结合和共轭研究
- 批准号:
1911335 - 财政年份:2019
- 资助金额:
$ 19.9万 - 项目类别:
Standard Grant
Earth's Electromagnetic Environment: Advancing Recent Discoveries in Auroral Plasma Radio Emission Research
地球电磁环境:推进极光等离子体无线电发射研究的最新发现
- 批准号:
1443338 - 财政年份:2015
- 资助金额:
$ 19.9万 - 项目类别:
Standard Grant
Collaborative Research: Remote Sensing of Electron Density Using Auroral Radio Emissions
合作研究:利用极光无线电发射遥感电子密度
- 批准号:
1147699 - 财政年份:2012
- 资助金额:
$ 19.9万 - 项目类别:
Continuing Grant
Collaborative Research: Applying the AGO Network to Energy Transfer in the Radiation Belts and Remote Sensing of Auroral Plasma Processes
合作研究:将AGO网络应用于辐射带能量传输和极光等离子体过程遥感
- 批准号:
1141817 - 财政年份:2012
- 资助金额:
$ 19.9万 - 项目类别:
Standard Grant
Outstanding Questions on Auroral Radiation Fine Structure
极光辐射精细结构的悬而未决的问题
- 批准号:
1043230 - 财政年份:2011
- 资助金额:
$ 19.9万 - 项目类别:
Standard Grant
Collaborative Research: Multi-instrument Studies of Auroral Plasma Radiation
合作研究:极光等离子体辐射的多仪器研究
- 批准号:
0838745 - 财政年份:2009
- 资助金额:
$ 19.9万 - 项目类别:
Standard Grant
Collaborative Research: PENGUIn - A High-Latitude Window to Geospace Dynamics
合作研究:PENGUIn——地球空间动力学的高纬度窗口
- 批准号:
0840669 - 财政年份:2009
- 资助金额:
$ 19.9万 - 项目类别:
Standard Grant
Collaborative Research: Auroral Radio Emissions Related to Substorms and Energetic Precipitation
合作研究:与亚暴和高能降水相关的极光无线电发射
- 批准号:
0753198 - 财政年份:2008
- 资助金额:
$ 19.9万 - 项目类别:
Standard Grant
Collaborative Research: Polar Experiment Network for Geospace Upper atmosphere Investigations (PENGUIn) - Advancing the Vision for Global Studies
合作研究:地球空间高层大气调查极地实验网络 (PENGUIn) - 推进全球研究的愿景
- 批准号:
0636798 - 财政年份:2007
- 资助金额:
$ 19.9万 - 项目类别:
Standard Grant
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相似海外基金
First Conjugate-Station Studies and Continued Satellite-Conjunction Studies of LF/MF/HF Auroral Radio Emissions at South Pole
南极 LF/MF/HF 极光无线电发射的首次共轭站研究和持续卫星联合研究
- 批准号:
2205753 - 财政年份:2022
- 资助金额:
$ 19.9万 - 项目类别:
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A study on MF/HF auroral radio emissions based on construction of new long-term continuous, high-resolution measurement instruments at multiple locations
基于在多个地点建造新型长期连续高分辨率测量仪器的中频/高频极光无线电发射研究
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Collaborative Research: Remote Sensing of Electron Density Using Auroral Radio Emissions
合作研究:利用极光无线电发射遥感电子密度
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合作研究:利用极光无线电发射遥感电子密度
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合作研究:与亚暴和高能降水相关的极光无线电发射
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0753451 - 财政年份:2008
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