Collaborative Research: Electron Acceleration and Emissions from the Solar Flare Termination Shock

合作研究:太阳耀斑终止激波的电子加速和发射

基本信息

  • 批准号:
    1735405
  • 负责人:
  • 金额:
    $ 16.88万
  • 依托单位:
  • 依托单位国家:
    美国
  • 项目类别:
    Standard Grant
  • 财政年份:
    2017
  • 资助国家:
    美国
  • 起止时间:
    2017-09-01 至 2020-08-31
  • 项目状态:
    已结题

项目摘要

This collaborative research project plans to make significant progress toward our understanding of one of the key problems in solar physics; i.e., the question of how electrons are accelerated within solar flares. Solar flares are the strongest explosions in the Solar System, and they provide sites for particle acceleration and high-energy emission. However, the question of exactly how this acceleration occurs remains unsolved. The project will combine two powerful numerical models that will enable the principal investigators (PIs) to simulate the physics over a wide range of scales from the large scale flares that produce shock waves down to the smallest scales where the particle acceleration occurs. This project will also support the training of the next generation of solar scientists. The PIs will involve both undergraduate and graduate students in the research, and funding is provided for a postdoctoral researcher for the project.In solar flares, a termination shock can develop when a high-speed outflow from the flare encounters magnetic loops in the solar atmosphere forming a standing shock wave that can accelerate particles to high energies. These shock waves had been predicted but never observed until recent X-ray and radio observations by one of the PIs (Chen). Motivated by this recent discovery, this project plans to investigate the dynamical evolution of termination shocks and their acceleration of electrons by combining, for the first time, two powerful numerical simulations: (1) large-scale magnetohydrodynamic (MHD) models of the dynamical evolution of a flare and (2) particle-in-cell kinetic and test-particle simulations for electron acceleration at the shock front. From the combined numerical model the PIs plan to generate synthetic hard X-ray emission and compare this emission with observations.
这个合作研究项目计划在我们理解太阳物理学中的一个关键问题上取得重大进展,即电子在太阳耀斑中如何加速的问题。太阳耀斑是太阳系中最强烈的爆炸,它们为粒子加速和高能发射提供了场所。然而,这种加速究竟是如何发生的问题仍然没有解决。该项目将结合两个强大的数值模型,使首席研究人员(PI)能够在从产生冲击波的大尺度耀斑到发生粒子加速的最小尺度的大范围内模拟物理。该项目还将支持对下一代太阳能科学家的培训。PIS将包括本科生和研究生参与研究,并为该项目的一名博士后研究员提供资金。在太阳耀斑中,当耀斑的高速外流与太阳大气中的磁环相遇时,可能会产生终止激波,形成驻留冲击波,从而将粒子加速到高能。这些冲击波已经被预测到了,但直到最近由其中一名PI(Chen)进行的X射线和无线电观测才被观测到。在这一最新发现的推动下,该项目计划通过首次结合两个强大的数值模拟来研究电子终止激波及其加速的动态演化:(1)耀斑动态演化的大尺度磁流体(MHD)模型和(2)激波前沿电子加速的胞内粒子动力学和测试粒子模拟。根据组合的数值模式,PI计划产生合成硬X射线发射,并将该发射与观测值进行比较。

项目成果

期刊论文数量(8)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)
Microwave and Hard X-Ray Observations of the 2017 September 10 Solar Limb Flare
  • DOI:
    10.3847/1538-4357/aad0ef
  • 发表时间:
    2018-08-10
  • 期刊:
  • 影响因子:
    4.9
  • 作者:
    Gary, Dale E.;Chen, Bin;Yu, Sijie
  • 通讯作者:
    Yu, Sijie
The Dynamical Behavior of Reconnection-driven Termination Shocks in Solar Flares: Magnetohydrodynamic Simulations
太阳耀斑中重新连接驱动的终止激波的动力学行为:磁流体动力学模拟
  • DOI:
    10.3847/1538-4357/aaeed3
  • 发表时间:
    2018-12
  • 期刊:
  • 影响因子:
    4.9
  • 作者:
    Shen Chengcai;Kong Xiangliang;Guo Fan;Raymond John C.;Chen Bin
  • 通讯作者:
    Chen Bin
Radio Spectroscopic Imaging of a Solar Flare Termination Shock: Split-band Feature as Evidence for Shock Compression
  • DOI:
    10.3847/1538-4357/ab3c58
  • 发表时间:
    2019-08
  • 期刊:
  • 影响因子:
    0
  • 作者:
    B. Chen 陈;Chengcai 彩 Shen 沈呈;K. Reeves;F. Guo 郭;Sijie 捷 Yu 余思
  • 通讯作者:
    B. Chen 陈;Chengcai 彩 Shen 沈呈;K. Reeves;F. Guo 郭;Sijie 捷 Yu 余思
Measurement of magnetic field and relativistic electrons along a solar flare current sheet
沿着太阳耀斑电流片测量磁场和相对论电子
  • DOI:
    10.1038/s41550-020-1147-7
  • 发表时间:
    2020-07-27
  • 期刊:
  • 影响因子:
    14.1
  • 作者:
    Chen, Bin;Shen, Chengcai;Kong, Xiangliang
  • 通讯作者:
    Kong, Xiangliang
Radio Spectral Imaging of an M8.4 Eruptive Solar Flare: Possible Evidence of a Termination Shock
  • DOI:
    10.3847/1538-4357/abe5a4
  • 发表时间:
    2021-04-01
  • 期刊:
  • 影响因子:
    4.9
  • 作者:
    Luo,Yingjie;Chen,Bin;Krucker,Sam
  • 通讯作者:
    Krucker,Sam
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Bin Chen其他文献

Another look at the moist baroclinic Ertel-Rossby invariant with mass forcing
再看看带有质量强迫的湿斜压 Ertel-Rossby 不变量
  • DOI:
  • 发表时间:
    2018
  • 期刊:
  • 影响因子:
    0
  • 作者:
    Shuai Yang;Shou-Ting Gao;Bin Chen
  • 通讯作者:
    Bin Chen
Results of Excimer Laser Ablation Combined with Drug-coated Balloon for Atherosclerotic Obliterans of Lower Extremity and Risk Factors for Loss of Primary Patency.
准分子激光消融联合药物涂层球囊治疗下肢动脉粥样硬化闭塞症的结果及失去主要通畅的危险因素。
  • DOI:
  • 发表时间:
    2022
  • 期刊:
  • 影响因子:
    1.5
  • 作者:
    Xiaolang Jiang;Xiaoyan Li;Bin Chen;Jun‐hao Jiang;Yun Shi;T. Ma;Chang;D. Guo;Xin Xu;Shuai Ju;W. Fu;Z. Dong
  • 通讯作者:
    Z. Dong
Targeting epigenetically maladapted vascular niche alleviates liver fibrosis in nonalcoholic steatohepatitis
靶向表观遗传适应不良的血管生态位可减轻非酒精性脂肪性肝炎的肝纤维化
  • DOI:
    10.1126/scitranslmed.abd1206
  • 发表时间:
    2021
  • 期刊:
  • 影响因子:
    17.1
  • 作者:
    Hua Zhang;Yongyuan Ma;Xinying Cheng;Dongbo Wu;Xingming Huang;Bin Chen;Yafeng Ren;Wei Jiang;Xiaoqiang Tang;Ting Bai;Yutian Chen;Yilin Zhao;Chunxue Zhang;Xia Xiao;Jing Liu;Yue Deng;Tinghong Ye;Lu Chen;Han-Min Liu;Scott L.Friedman;Liping Chen;Bi-Sen Ding;Zho
  • 通讯作者:
    Zho
群在dendrite上作用的Auslander-Yorke混沌
A new exponentially weighted moving average control chart for monitoring the coefficient of variation
用于监控变异系数的新指数加权移动平均控制图
  • DOI:
    10.1016/j.cie.2014.09.027
  • 发表时间:
    2014-12
  • 期刊:
  • 影响因子:
    7.9
  • 作者:
    Jiujun Zhang;Li Zhonghua;Bin Chen;Zhaojun Wang
  • 通讯作者:
    Zhaojun Wang

Bin Chen的其他文献

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{{ truncateString('Bin Chen', 18)}}的其他基金

MRI RI-Track 2: Development of the Expanded Owens Valley Solar Array (EOVSA)-15--Major Upgrade of a Community Facility for Solar and Space Weather Physics
MRI RI-轨道 2:扩展欧文斯谷太阳能电池阵列 (EOVSA)-15 的开发——太阳能和空间天气物理社区设施的重大升级
  • 批准号:
    2320478
  • 财政年份:
    2023
  • 资助金额:
    $ 16.88万
  • 项目类别:
    Standard Grant
Collaborative Research: SHINE: Where Are Particles Accelerated in Coronal Jets?
合作研究:SHINE:日冕喷流中的粒子在哪里加速?
  • 批准号:
    2229338
  • 财政年份:
    2023
  • 资助金额:
    $ 16.88万
  • 项目类别:
    Standard Grant
Collaborative Research: Achieving a New Understanding of Solar Flare Termination Shocks
合作研究:对太阳耀斑终止激波有了新的认识
  • 批准号:
    2108853
  • 财政年份:
    2021
  • 资助金额:
    $ 16.88万
  • 项目类别:
    Continuing Grant
Structure and thermal elastic properties of calcium silicate perovskite
硅酸钙钛矿的结构与热弹性性能
  • 批准号:
    2127807
  • 财政年份:
    2021
  • 资助金额:
    $ 16.88万
  • 项目类别:
    Standard Grant
Laboratory Technician Support: Experimental Mineral Physics and Petrology Facilities at the University of Hawaii at Manoa
实验室技术人员支持:夏威夷大学马诺阿分校的实验矿物物理和岩石学设施
  • 批准号:
    1829273
  • 财政年份:
    2018
  • 资助金额:
    $ 16.88万
  • 项目类别:
    Continuing Grant
Collaborative Research: SHINE--Magnetic Energy Release During Solar Eruptions - From Large to Small Scales
合作研究:SHINE——太阳喷发期间的磁能释放——从大尺度到小尺度
  • 批准号:
    1723436
  • 财政年份:
    2017
  • 资助金额:
    $ 16.88万
  • 项目类别:
    Standard Grant
CAREER: Probing Energy Release in Solar Explosive Events with New Generation Radio Telescopes
职业:用新一代射电望远镜探测太阳爆炸事件中的能量释放
  • 批准号:
    1654382
  • 财政年份:
    2017
  • 资助金额:
    $ 16.88万
  • 项目类别:
    Continuing Grant
CAREER: Elasticity and Lattice Dynamics of Iron Alloys under Earth's Core Conditions
职业:地球核心条件下铁合金的弹性和晶格动力学
  • 批准号:
    1555388
  • 财政年份:
    2016
  • 资助金额:
    $ 16.88万
  • 项目类别:
    Continuing Grant
CSEDI Collaborative Research: Experimental and Theoretical Investigations on the Elastic and Viscoelastic Properties of Fe-Ni-C Liquids
CSEDI合作研究:Fe-Ni-C液体弹性和粘弹性的实验和理论研究
  • 批准号:
    1565708
  • 财政年份:
    2016
  • 资助金额:
    $ 16.88万
  • 项目类别:
    Continuing Grant
CDI-Type I: Collaborative Research: Development of computational algorithms and analysis tools for molecular-level understanding of complex atmospheric nucleation processes
CDI-I 型:合作研究:开发计算算法和分析工具,以在分子水平上理解复杂的大气成核过程
  • 批准号:
    1052015
  • 财政年份:
    2010
  • 资助金额:
    $ 16.88万
  • 项目类别:
    Standard Grant

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