Acquisition of Ultra High Speed Framing Camera to be used for Investigations of Laboratory Simulations of Solar Prominence Dynamics
采购超高速分幅相机,用于研究日珥动力学的实验室模拟
基本信息
- 批准号:0114545
- 负责人:
- 金额:$ 19.72万
- 依托单位:
- 依托单位国家:美国
- 项目类别:Standard Grant
- 财政年份:2001
- 资助国家:美国
- 起止时间:2001-09-01 至 2003-08-31
- 项目状态:已结题
- 来源:
- 关键词:
项目摘要
The investigators will purchase an advanced high-speed camera to make sixteen frame movies of single plasma "shots". The main objective is to be able to follow magnetic reconnection and the propagation of ripples of magnetic twist (such as Alfven waves) away from regions of reconnection. The framing rate will be between 8 million and 200 million frames per second. Shot-to-shot reproducibility will no longer be a constraint because the entire fine structure evolution will be captured in a single shot. Data throughput will be increased 16-fold enabling many more experiments and investigation of many important phenomena not being pursued at present. Simulated solar prominences in the laboratory have recently been demonstrated using a unique, specially designed experimental facility at Caltech. The facility uses pulsed power plasma technology to produce a short-lived plasma (10 microseconds) with large magnetic fields (several kilogauss), high currents (tens of kiloamps), and modest dimensions (tens of centimeters). This plasma has the morphology and dynamics of a solar prominence. A program is underway to investigate the topological evolution of these simulated prominences. Topological evolution involves the breaking and reconnection of magnetic field lines and is believed to be a critical process in solar prominence eruptions. The present method for diagnosing the solar prominence simulation experiments uses a single-frame high-speed digital camera, that is a camera that takes a single photograph at a time. The technique consists of creating a sequence of identical plasma shots and then making a single ten nanosecond photo of each shot, but with increasing time offsets of a few hundred nanoseconds. The shot-to-shot reproducibility is sufficient to follow the gross variation in morphology, but not the details. Because it takes about 2 minutes to recharge the pulse power capacitor banks between plasma shots, this single-shot accumulation technique is both tedious and time consuming.
调查人员将购买一台先进的高速相机,制作单个等离子体“镜头”的16部框架电影。 主要目的是能够遵循磁性旋转(例如Alfven波)的连接的传播,从重新连接区域远离。框架率为每秒800万至2亿帧。射击的可重复性将不再是限制,因为整个精细结构演变将被单镜头捕获。数据吞吐量将增加16倍,以实现更多实验,并研究目前尚未追求许多重要现象。最近,使用Caltech的独特,专门设计的实验设施证明了实验室中的模拟太阳突出。该设施使用脉冲功率等离子体技术来生产具有较大磁场(几毫秒)(几千摩斯),高电流(数十千兆)和适度尺寸(数十厘米)的短寿命等离子体(10微秒)。该等离子体具有太阳突出的形态和动力学。正在进行一个计划,以研究这些模拟突出的拓扑演变。拓扑演化涉及磁场线的破坏和重新连接,被认为是太阳突出喷发中的关键过程。目前诊断太阳突出模拟实验的方法使用了单帧的高速数码相机,该摄像头一次拍摄一张照片。该技术包括创建一系列相同的等离子体镜头,然后制作每张镜头的十纳秒照片,但随着时间的偏移增加了几百纳秒。射击的可重复性足以遵循形态的总变化,但细节不足。因为在等离子体镜头之间为脉冲电容器库充电大约需要2分钟,所以这种单发积累技术既乏味又耗时。
项目成果
期刊论文数量(0)
专著数量(0)
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会议论文数量(0)
专利数量(0)
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Paul Bellan其他文献
On the jets, kinks, and spheromaks formed by a planar magnetized coaxial gun (12 pages)
平面磁化同轴枪形成的射流、扭结和球体(12 页)
- DOI:
10.1063/1.1850921 - 发表时间:
2004 - 期刊:
- 影响因子:2.2
- 作者:
L. Marrelli;L. Frassinetti;Darren Craig;J. Sarff;Scott Hsu;Paul Bellan;Richard L. Berger;E. Valeo;R. Torasso;Eliezer Hameiri - 通讯作者:
Eliezer Hameiri
Enrichment of the Dust-to-Gas Mass Ratio in Bondi/Jeans Accretion/Cloud Systems due to Unequal Changes in Dust and Gas Incoming Velocities
由于灰尘和气体进入速度的不均匀变化导致 Bondi/Jeans 吸积/云系统中灰尘与气体质量比的富集
- DOI:
10.1086/533483 - 发表时间:
2008 - 期刊:
- 影响因子:0
- 作者:
Paul Bellan - 通讯作者:
Paul Bellan
Fundamentals of Plasma Physics: Intuitive method for vector calculus identities
- DOI:
10.1017/cbo9780511807183.019 - 发表时间:
2006-04 - 期刊:
- 影响因子:33.6
- 作者:
Paul Bellan - 通讯作者:
Paul Bellan
Dust-driven Dynamos in Accretion Disks
吸积盘中的灰尘驱动发电机
- DOI:
10.1086/591244 - 发表时间:
2008 - 期刊:
- 影响因子:0
- 作者:
Paul Bellan - 通讯作者:
Paul Bellan
Acceleration of charged particles to extremely large energies by a sub-Dreicer electric field
通过亚德雷瑟电场将带电粒子加速到极大的能量
- DOI:
10.1063/1.5081716 - 发表时间:
2019 - 期刊:
- 影响因子:2.2
- 作者:
Ryan S. Marshall;Paul Bellan - 通讯作者:
Paul Bellan
Paul Bellan的其他文献
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{{ truncateString('Paul Bellan', 18)}}的其他基金
Determining the Ice Phase, Nucleation Process, and Electromagnetic Interaction Properties of the Ice Grains in an Ice Dusty Plasma
确定冰尘等离子体中冰粒的冰相、成核过程和电磁相互作用特性
- 批准号:
2308558 - 财政年份:2023
- 资助金额:
$ 19.72万 - 项目类别:
Continuing Grant
Determining How Plasma Spontaneously Develops a Localized Hot Spot That Radiates X-rays and Produces Related Dramatic Phenomena
确定等离子体如何自发形成辐射 X 射线的局部热点并产生相关的戏剧性现象
- 批准号:
2105492 - 财政年份:2021
- 资助金额:
$ 19.72万 - 项目类别:
Standard Grant
Determining the Cross-Scale Coupling whereby Magnetohydrodynamics (MHD) Solar Eruptions Produce Energetic Electrons and X-Rays
确定磁流体动力学 (MHD) 太阳喷发产生高能电子和 X 射线的跨尺度耦合
- 批准号:
1914599 - 财政年份:2019
- 资助金额:
$ 19.72万 - 项目类别:
Standard Grant
Development of Laser Induced Fluorescence as a Diagnostic for Measuring Neutral, Ion, and Molecule Particle Fluxes in the PK-4 Experiment
开发激光诱导荧光作为 PK-4 实验中测量中性、离子和分子粒子通量的诊断方法
- 批准号:
1740655 - 财政年份:2017
- 资助金额:
$ 19.72万 - 项目类别:
Continuing Grant
Collaborative Research: SHINE: Laboratory, Observational, and Modeling Investigations of the Torus Instability and Associated Solar Corona Eruptive Phenomena
合作研究:SHINE:环面不稳定性和相关日冕喷发现象的实验室、观测和建模研究
- 批准号:
1348393 - 财政年份:2014
- 资助金额:
$ 19.72万 - 项目类别:
Continuing Grant
SHINE: Improving Understanding of Solar Corona Dynamics Using Laboratory Simulations of Coronal Loops
SHINE:利用日冕环的实验室模拟提高对日冕动力学的理解
- 批准号:
1059519 - 财政年份:2011
- 资助金额:
$ 19.72万 - 项目类别:
Continuing Grant
Non-equilibrium Magnetohydrodynamic Behavior of Plasmas Having Complex, Evolving Morphology
具有复杂、演化形态的等离子体的非平衡磁流体动力学行为
- 批准号:
0901916 - 财政年份:2009
- 资助金额:
$ 19.72万 - 项目类别:
Standard Grant
SHINE: Improving Understanding of Solar Corona Dynamics Using Laboratory Simulations of Coronal Loops
SHINE:利用日冕环的实验室模拟提高对日冕动力学的理解
- 批准号:
0746644 - 财政年份:2008
- 资助金额:
$ 19.72万 - 项目类别:
Continuing Grant
Collaborative Research: Testing a New Concept for the Long-term Build-up to Coronal Mass Ejections
合作研究:测试日冕物质抛射长期积累的新概念
- 批准号:
0837910 - 财政年份:2008
- 资助金额:
$ 19.72万 - 项目类别:
Continuing Grant
Investigation of How Microscopic Stochastic Particle Motion Affects Macroscropic Fluid Behavior in a Magnetized Plasma
研究微观随机粒子运动如何影响磁化等离子体中的宏观流体行为
- 批准号:
9413046 - 财政年份:1995
- 资助金额:
$ 19.72万 - 项目类别:
Continuing Grant
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