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
基本信息
- 批准号:2308558
- 负责人:
- 金额:$ 98.38万
- 依托单位:
- 依托单位国家:美国
- 项目类别:Continuing Grant
- 财政年份:2023
- 资助国家:美国
- 起止时间:2023-08-01 至 2026-07-31
- 项目状态:未结题
- 来源:
- 关键词:
项目摘要
The award supports an experimental study of water ice grain formation in a weakly ionized plasma environment. Plasma - a gas containing free electrons and ions - can be weakly ionized so that the gas is almost all neutral atoms and molecules with only one part in a million consisting of the electrically charged particles. This experimental research program will study a weakly-ionized plasma where the neutral gas is arranged to be extremely cold, such as -300F. When a small amount of water vapor is injected into such plasma, it is found that tiny grains of ice spontaneously form, become electrically charged, and are suspended in the plasma. The ice grains range in size from nanometers to hundreds of micrometers depending on experimental conditions. The new study will provide information relevant to situations that occur in nature such as the protoplanetary disk that existed in the early stage of solar system evolution, the diffuse rings of Saturn, and terrestrial noctilucent clouds that can form at 50-mile altitudes in polar regions.The project has two main goals. The first is to determine how the ice grain infrared absorption spectrum varies with temperature. At the extremely cold temperatures found in many astrophysical situations, ice can be in an amorphous phase and so have a different infrared absorption spectrum from the crystalline ice of ordinary experience. The second main goal is determining why and how ice nucleates in a plasma. For terrestrial atmospheric conditions it is well established that ice nucleation requires a core of non-ice solid material, such as carbon or silicate, on which ice forms as a coating. However, laboratory plasma experiments do not contain any non-ice material and preliminary evidence is that the weakly-ionized plasma catalyzes ice nucleation. The investigation will explore how the weakly-ionized plasma environment may enable ice nucleation and will be guided by a theoretical prediction that high-energy plasma electrons, a tiny minority of all free electrons, may play a key role in the process.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.
该奖项支持在弱电离等离子体环境中形成水冰粒的实验研究。 等离子体-一种含有自由电子和离子的气体-可以被弱电离,使得气体几乎都是中性原子和分子,只有百万分之一的带电粒子。该实验研究计划将研究弱电离等离子体,其中中性气体被布置为极冷,例如-300 F。 当少量的水蒸气被注入到这样的等离子体中时,人们发现微小的冰粒自发地形成,变得带电,并悬浮在等离子体中。 根据实验条件,冰粒的大小从纳米到数百微米不等。这项新研究将提供与自然界中发生的情况相关的信息,如太阳系演化早期存在的原行星盘,土星的扩散环,以及极地地区50英里高度形成的陆地日冕云。该项目有两个主要目标。首先是确定冰粒红外吸收光谱如何随温度变化。在许多天体物理学环境中发现的极冷温度下,冰可以处于非晶相,因此具有与普通经验中的结晶冰不同的红外吸收光谱。 第二个主要目标是确定冰为什么以及如何在等离子体中成核。对于陆地大气条件,已经确定的是,冰成核需要非冰固体材料的核心,例如碳或硅酸盐,冰在其上形成作为涂层。 然而,实验室等离子体实验不包含任何非冰材料,初步证据是弱电离等离子体催化冰成核。 该研究将探索弱电离等离子体环境如何使冰成核,并将以理论预测为指导,即高能等离子体电子(所有自由电子中的极少数)可能在该过程中发挥关键作用。该奖项反映了NSF的法定使命,并被认为值得通过使用基金会的智力价值和更广泛的影响审查标准进行评估来支持。
项目成果
期刊论文数量(0)
专著数量(0)
科研奖励数量(0)
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 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:
$ 98.38万 - 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:
$ 98.38万 - 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:
$ 98.38万 - 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:
$ 98.38万 - 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:
$ 98.38万 - 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:
$ 98.38万 - 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:
$ 98.38万 - 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:
$ 98.38万 - 项目类别:
Continuing Grant
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
- 批准号:
0114545 - 财政年份:2001
- 资助金额:
$ 98.38万 - 项目类别:
Standard 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:
$ 98.38万 - 项目类别:
Continuing Grant
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