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Diffusion tensor imaging of optic nerve and optic radiation in primary chronic angle-closure glaucoma using 3T magnetic resonance imaging 被引量:10
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作者 Qiu-Juan Zhang Dong Wang +2 位作者 Zhi-Lan Bai Bai-Chao Ren Xiao-Hui Li 《International Journal of Ophthalmology(English edition)》 SCIE CAS 2015年第5期975-979,共5页
AIM: To evaluate the value of quantitative diffusion tensor imaging (DTI) in assessing the axonal and myelin damage of the optic nerves and optic radiations in patients with chronic primary angle -closure glaucoma (PA... AIM: To evaluate the value of quantitative diffusion tensor imaging (DTI) in assessing the axonal and myelin damage of the optic nerves and optic radiations in patients with chronic primary angle -closure glaucoma (PACG) by using high -field magnetic resonance (MR) imaging (3T). METHODS: Twenty patients with bilateral chronic PACG and twenty age - and sex matched disease -free control subjects were enrolled. Conventional MRI and DTI were performed on all subjects using 3T MR scanner. Mean diffusivity (MD), fractional anisotropy (FA), axial diffusivities (AD) and radial diffusivities (RD) of each optic nerve and each optic radiation were measured by using post -processing software of DTI studio 2.3, and then compared between left eyes and right eyes and between patients group and control group. The pairedsample t- test were used. RESULTS: There was no abnormality in the shape and signal intensity of the optic nerves and optic radiations in patients group and control group on the conventional MRI. No significant differences were observed in the FA, MD, AD and RD between the right and left optic nerves and optic radiations within patients group and control group (P>0.05). The optic nerves and optic radiations of patients with chronic PACG, as compared with control subjects, had significantly higher MD, AD, RD and significantly lower FA (P<0.05). CONCLUSION: The diffusivity of optic nerves and optic radiations in chronic PACG group showed abnormal and diffusivity parameters could be used markers of axonal and myelin injury in glaucoma. 展开更多
关键词 primary angle-closure glaucoma CHRONIC optic nerve and optic radiation diffusion tensor imaging magnetic resonance imaging
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Radiation belt electron scattering by whistler-mode chorus in the Jovian magnetosphere: Importance of ambient and wave parameters 被引量:3
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作者 BinBin Ni Jing Huang +6 位作者 YaSong Ge Jun Cui Yong Wei XuDong Gu Song Fu Zheng Xiang ZhengYu Zhao 《Earth and Planetary Physics》 2018年第1期1-14,共14页
Whistler-mode chorus waves are regarded as an important acceleration mechanism contributing to the formation of relativistic and ultra-relativistic electrons in the Jovian radiation belts. Quantitative determination o... Whistler-mode chorus waves are regarded as an important acceleration mechanism contributing to the formation of relativistic and ultra-relativistic electrons in the Jovian radiation belts. Quantitative determination of the chorus wave driven electron scattering effect in the Jovian magnetosphere requires detailed information of both ambient magnetic field and plasma density and wave spectral property, which however cannot be always readily acquired from observations of existed missions to Jupiter. We therefore perform a comprehensive analysis of the sensitivity of chorus induced electron scattering rates to ambient magnetospheric and wave parameters in the Jovian radiation belts to elaborate to which extent the diffusion coefficients depend on a number of key input parameters. It is found that quasi-linear electron scattering rates by chorus can be strongly affected by the ambient magnetic field intensity, the wave latitudinal coverage, and the peak frequency and bandwidth of the wave spectral distribution in the Jovian magnetosphere, while they only rely slightly on the background plasma density profile and the peak wave normal angle, especially when the wave emissions are confined at lower latitudes. Given the chorus wave amplitude, chorus induced electron scattering rates strongly depend on Jovian L-shell to exhibit a tendency approximately proportional to L_J^3. Our comprehensive analysis explicitly demonstrates the importance of reliable information of both the ambient magnetospheric state and wave distribution property to understanding the dynamic electron evolution in the Jovian radiation belts and therefore has implications for future mission planning to explore the extreme particle radiation environment of Jupiter and its satellites. 展开更多
关键词 Jovian radiation BELTS whistler-mode CHORUS resonant wave-particle interactions magnetospheric state
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光栅—谐振腔复合结构中的史密斯—帕塞尔辐射(英文) 被引量:3
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作者 孟现柱 王明红 任忠民 《红外与毫米波学报》 SCIE EI CAS CSCD 北大核心 2016年第1期21-24,共4页
提出了光栅—谐振腔复合结构.利用光学理论和粒子模拟方法研究了这种光栅—谐振腔复合结构中的史密斯—帕塞尔辐射的输出特性.结果显示:利用这种装置可以产生太赫兹波段的可调谐相干史密斯—帕塞尔辐射.这种光栅—谐振腔复合结构具有下... 提出了光栅—谐振腔复合结构.利用光学理论和粒子模拟方法研究了这种光栅—谐振腔复合结构中的史密斯—帕塞尔辐射的输出特性.结果显示:利用这种装置可以产生太赫兹波段的可调谐相干史密斯—帕塞尔辐射.这种光栅—谐振腔复合结构具有下列优点:它可以把一定发射角和任意方位角的史密斯—帕塞尔辐射同相位反馈到电子束,对电子束进行调制. 展开更多
关键词 电子物理学 史密斯—帕塞尔辐射 粒子模拟 光栅—谐振腔复合结构
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一种可能的反常空气簇射
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作者 张希芝 《郑州大学学报(理学版)》 CAS 1994年第2期35-37,共3页
在空气簇射实验中,已观测到来自x-射线双脉冲星的超高能和甚高能辐射事例,其中的一些实验,原初辐射显示强子的性质,而不具有光子的性质,这些强子同目前巳知的粒子不符,本文对特征大小约为10fm正负电子系统的一些窄的,长寿... 在空气簇射实验中,已观测到来自x-射线双脉冲星的超高能和甚高能辐射事例,其中的一些实验,原初辐射显示强子的性质,而不具有光子的性质,这些强子同目前巳知的粒子不符,本文对特征大小约为10fm正负电子系统的一些窄的,长寿命的共振态引起反常空气簇射的可能性进行了考察. 展开更多
关键词 空气簇射 反常行为 共振粒子 原初辐射
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Recent progress on ULF wave and its interactions with energetic particles in the inner magnetosphere 被引量:16
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作者 Theodore A. FRITZ 《Science China(Technological Sciences)》 SCIE EI CAS 2008年第10期1620-1625,共6页
The global distribution properties of Ultra Low Frequency wave (ULF) in the inner magnetospgere and its interactions with energetic particles, such as the wave-particle resonance, modulation, and particle acceleration... The global distribution properties of Ultra Low Frequency wave (ULF) in the inner magnetospgere and its interactions with energetic particles, such as the wave-particle resonance, modulation, and particle acceleration, are active topics in space physics research. These problems are fundamentally important issues to understand the energy transport from the solar wind into the magnetosphere. In this paper we briefly reviewed the recent research progress on ULF wave and its interactions with energetic particles in the inner magnetosphere; furthermore, we suggested some open questions for future study. 展开更多
关键词 radiation BELT particlE particlE acceleration ULF wave compressional MODE cavity MODE poloidal MODE TOROIDAL MODE Field Line resonance (FLR) ENERGETIC particles modulation
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Mathematical Overview of Hypersphere World-Universe Model 被引量:6
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作者 Vladimir S. Netchitailo 《Journal of High Energy Physics, Gravitation and Cosmology》 2017年第3期415-437,共23页
The Hypersphere World-Universe Model (WUM) provides a mathematical framework that allows calculating the primary cosmological parameters of the World which are in good agreement with the most recent measurements and o... The Hypersphere World-Universe Model (WUM) provides a mathematical framework that allows calculating the primary cosmological parameters of the World which are in good agreement with the most recent measurements and observations. WUM explains the experimental data accumulated in the field of Cosmology and Astroparticle Physics over the last decades: the age of the World and critical energy density;the gravitational parameter and Hubble’s parameter;temperatures of the cosmic microwave background radiation and the peak of the far-infrared background radiation;the concentration of intergalactic plasma and time delay of Fast Radio Bursts. Additionally, the model predicts masses of dark matter particles, photons, and neutrinos;proposes new types of particle interactions (Super Weak and Extremely Weak);shows inter-connectivity of primary cosmological parameters of the World. WUM proposes to introduce a new fundamental parameter Q in the CODATA internationally recommended values. This paper is the summary of the mathematical results obtained in [1]-[4]. 展开更多
关键词 HYPERSPHERE World-Universe Model primary COSMOLOGICAL Parameters Medium of the World Macroobjects Structure Gravitoelectromagnetism Dark Matter particles Intergalactic Plasma Microwave BACKGROUND radiation FAR-INFRARED BACKGROUND radiation Fast Radio BURSTS Emergent Phenomena CODATA
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Hypersphere World-Universe Model 被引量:3
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作者 Vladimir S. Netchitailo 《Journal of High Energy Physics, Gravitation and Cosmology》 2021年第2期915-941,共27页
Dirac’s themes were the unity and beauty of Nature. He identified three revolutions in modern physics: Relativity, Quantum Mechanics and Cosmology. In his opinion: “<i>The new cosmology will probably turn out ... Dirac’s themes were the unity and beauty of Nature. He identified three revolutions in modern physics: Relativity, Quantum Mechanics and Cosmology. In his opinion: “<i>The new cosmology will probably turn out to be philosophically even more revolutionary than relativity or the quantum theory, perhaps looking forward to the current bonanza in cosmology, where precise observations on some of the most distant objects in the universe are shedding light on the nature of reality, on the nature of matter and on the most advanced quantum theories</i>” [Farmelo, G. (2009) The Strangest Man. The Hidden Life of Paul Dirac, Mystic of the Atom. Basic Books, Britain, 661 p]. In 1937, Paul Dirac proposed the Large Number Hypothesis and the Hypothesis of the variable gravitational “constant”;and later added the notion of continuous creation of Matter in the World. The developed Hypersphere World-Universe Model (WUM) follows these ideas, albeit introducing a different mechanism of matter creation. In this paper, we show that WUM is a natural continuation of Classical Physics and it can already serve as a basis for a New Cosmology proposed by Paul Dirac. 展开更多
关键词 Hypersphere World-Universe Model Law of Conservation of Angular Momentum Dark Epoch Rotational Fission Luminous Epoch Dark Matter particles Macroobject Shell Model Dark Matter Core Medium of the World Dark Matter Fermi Bubbles Galactic Wind Solar Wind Gravitational Bursts Intergalactic Plasma Macroobjects Supremacy of Matter Gravitomagnetic parameter Impedance Energy Density Gravitational Parameter Hubble’s Parameter Temperature of Microwave Background radiation Inter-Connectivity of primary Cosmological Parameters Dark Matter Reactor
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Hypersphere World-Universe Model: Evolution of the World 被引量:2
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作者 Vladimir S. Netchitailo 《Journal of High Energy Physics, Gravitation and Cosmology》 2021年第2期508-530,共23页
The main objective of this paper is to discuss the Evolution of a 3D Finite World (that is a Hypersphere of a 4D Nucleus of the World) from the Beginning up to the present Epoch in frames of World-Universe Model (WUM)... The main objective of this paper is to discuss the Evolution of a 3D Finite World (that is a Hypersphere of a 4D Nucleus of the World) from the Beginning up to the present Epoch in frames of World-Universe Model (WUM). WUM is the only cosmological model in existence that is consistent with the Law of Conservation of Angular Momentum. To be consistent with this Fundamental Law, WUM introduces Dark Epoch (spanning from the Beginning of the World for 0.45 billion years) when only Dark Matter (DM) Macroobjects (MOs) existed, and Luminous Epoch (ever since for 13.77 billion years) when Luminous MOs emerged due to Rotational Fission of Overspinning DM Superclusters’ Cores and self-annihilation of Dark Matter Particles (DMPs). WUM envisions that DM is created by the Universe in the 4D Nucleus of the World. Dark Matter Particles (DMPs) carry new DM into the 3D Hypersphere World. Luminous Matter is a byproduct of DMPs self-annihilation. By analogy with 3D ball, which has two-dimensional sphere surface (that has surface energy), we can imagine that the 3D Hypersphere World has a “Surface Energy” of the 4D Nucleus. WUM solves a number of physical problems in contemporary Cosmology and Astrophysics through DMPs and their interactions: <b>Angular Momentum problem</b> in birth and subsequent evolution of Galaxies and Extrasolar systems—how do they obtain it;<b>Fermi Bubbles</b>—two large structures in gamma-rays and X-rays above and below Galactic center;<b>Missing Baryon problem</b> related to the fact that the observed amount of baryonic matter did not match theoretical predictions. WUM reveals <b>Inter-Connectivity of Primary Cosmological Parameters</b> and calculates their values, which are in good agreement with the latest results of their measurements. In 2013, WUM predicted the values of the following Cosmological parameters: gravitational, concentration of intergalactic plasma, and the minimum energy of photons, which were experimentally confirmed in 2015-2018. “<i>The Discovery of a Supermassive Compact Object at the Centre of Our Galaxy</i>” (Nobel Prize in Physics 2020) made by Prof. R. Genzel and A. Ghez is a confirmation of one of the most important predictions of WUM in 2013: “<i>Macroobjects of the World have cores made up of the discussed DM particles. Other particles, including DM and baryonic matter, form shells surrounding the cores</i>”. 展开更多
关键词 Hypersphere World-Universe Model Law of Conservation of Angular Momentum Dark Epoch Rotational Fission Luminous Epoch Dark Matter particles Macroobject Shell Model Dark Matter Core Medium of the World Dark Matter Fermi Bubbles Galactic Wind Solar Wind Gamma-Ray Bursts Gravitational Bursts Intergalactic Plasma Cosmological Time Solar Time Macroobjects Supremacy of Matter Gravitomagnetic Parameter Impedance Energy Density Gravitational Parameter Hubble’s Parameter Temperature of Microwave Background radiation Inter-Connectivity of primary Cosmological Parameters Dark Matter Reactor
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基于微型谐振腔的史密斯-帕赛尔自由电子激光 被引量:3
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作者 孟现柱 王明红 +1 位作者 孙桂芳 吴立恒 《聊城大学学报(自然科学版)》 2018年第4期48-51,共4页
研究了一种由电子枪、微谐振腔、金属光栅和集电极组成的新型史密斯-帕赛尔自由电子激光.利用PIC三维模拟,讨论了该装置的特点.发现在合理的电子能量和光栅参数下,该装置可以产生THz频率范围内的相干高功率脉冲SPR.研究结果表明,当电子... 研究了一种由电子枪、微谐振腔、金属光栅和集电极组成的新型史密斯-帕赛尔自由电子激光.利用PIC三维模拟,讨论了该装置的特点.发现在合理的电子能量和光栅参数下,该装置可以产生THz频率范围内的相干高功率脉冲SPR.研究结果表明,当电子束能量E=50keV,电子束电流I=10A时,光栅周期L=0.3mm时,可以得到功率在4 000W左右、脉冲为0.25ns的514.643GHz的太赫兹辐射. 展开更多
关键词 太赫兹 史密斯帕赛尔辐射 PIC模拟 谐振腔 光栅
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From the Beginning of the World to the Beginning of Life on Earth 被引量:3
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作者 Vladimir S. Netchitailo 《Journal of High Energy Physics, Gravitation and Cosmology》 2021年第4期1503-1523,共21页
Hypersphere World-Universe Model (WUM) is, in fact, a Paradigm Shift in Cosmology [1]. In this paper, we provide seven Pillars of WUM: Medium of the World;Inter-Connectivity of Primary Cosmological Parameters;Creation... Hypersphere World-Universe Model (WUM) is, in fact, a Paradigm Shift in Cosmology [1]. In this paper, we provide seven Pillars of WUM: Medium of the World;Inter-Connectivity of Primary Cosmological Parameters;Creation of Matter;Multicomponent Dark Matter;Macroobjects;Volcanic Rotational Fission;Dark Matter Reactors. We describe the evolution of the World from the Beginning up to the birth of the Solar System and discuss the condition of the Early Earth before the beginning of life on it. 展开更多
关键词 Hypersphere World-Universe Model Law of Conservation of Angular Momentum Dark Epoch Volcanic Rotational Fission Luminous Epoch Dark Matter particles Macroobject Shell Model Dark Matter Core Medium of the World Dark Matter Fermi Bubbles Galactic Wind Solar Wind Intergalactic Plasma Macroobjects Gravitomagnetic Parameter Impedance Energy Density Gravitational Parameter Hubble’s Parameter Temperature of Microwave Background radiation Inter-Connectivity of primary Cosmological Parameters Dark Matter Reactor Early Earth Formation of Earth Origin of Moon Continental Crust of Earth Earth’s Atmosphere and Oceans Origin of Life
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场向传播的内磁层哨声波对辐射带高能电子的共振扩散 被引量:4
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作者 倪彬彬 赵正予 +1 位作者 顾旭东 汪枫 《物理学报》 SCIE EI CAS CSCD 北大核心 2008年第12期7937-7949,共13页
基于高斯分布的哨声波谱密度分布、偶极子背景磁场模型以及建立在卫星观测数据基础上的半经验电子密度纬度分布模型,对于等离子体层顶以外区域(4≤L≤7),计算了准线性当地及弹跳平均电子共振扩散系数,并估算了与磁层哨声波回旋共振导致... 基于高斯分布的哨声波谱密度分布、偶极子背景磁场模型以及建立在卫星观测数据基础上的半经验电子密度纬度分布模型,对于等离子体层顶以外区域(4≤L≤7),计算了准线性当地及弹跳平均电子共振扩散系数,并估算了与磁层哨声波回旋共振导致的辐射带电子损失及加速时间尺度.结果表明,波粒共振相互作用区域取决于电子能量、波谱分布、电子赤道抛射角以及当地电子密度及背景磁场.哨声波共振频率除了与以上5个参量有关外,还与地磁纬度有关.赤道哨声波主要影响较低能量辐射带电子的加速,中高纬度哨声波主要作用于较高能量辐射带电子的沉降损失.对于较低能量(约200keV)的辐射带电子,磁层哨声波可以在几个小时内使之沉降,对于较高能量(约1MeV)的电子,则需要一到数天;对低能量(约200keV)电子的加热可以在数小时内完成,回旋加速较高能量(约1MeV)电子一般则需要3—4d.电子密度分布的改变能够明显影响电子共振损失时间尺度,但是对电子共振加速时间尺度的作用很小.随着电子密度增强幅度随纬度的上升而增大,电子共振损失时间尺度会随之增大,但是电子共振加速时间尺度基本上不变化.另外,哨声波幅度及频谱随L及纬度的分布也显著影响它对辐射带电子的共振扩散效果,这些作用一般要大于电子密度分布变化带来的影响. 展开更多
关键词 共振波粒相互作用 地球辐射带 哨声波 回旋共振加速及散射沉降
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典型甚低频电磁波对辐射带高能电子的散射损失效应 被引量:2
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作者 罗旭东 牛胜利 左应红 《物理学报》 SCIE EI CAS CSCD 北大核心 2015年第6期406-413,共8页
辐射带中高能电子与空间甚低频电磁波由于波粒共振相互作用发生投掷角散射,进而沉降入稠密大气而损失.为研究甚低频电磁波对辐射带中高能电子的散射作用机制,本文基于准线性扩散理论,利用库仑作用和波粒共振相互作用扩散系数的物理模型... 辐射带中高能电子与空间甚低频电磁波由于波粒共振相互作用发生投掷角散射,进而沉降入稠密大气而损失.为研究甚低频电磁波对辐射带中高能电子的散射作用机制,本文基于准线性扩散理论,利用库仑作用和波粒共振相互作用扩散系数的物理模型,得到了两组典型甚低频电磁波与高能电子波粒共振相互作用的赤道投掷角弹跳周期平均扩散系数,并分析了甚低频电磁波共振散射作用与大气库仑散射作用对不同磁壳及不同能量的辐射带电子扩散损失的影响规律.以磁壳参数L=2.2,能量E=0.5 Me V的辐射带电子作为算例,采用有限差分方法数值求解扩散方程,计算分析了电子单向通量和全向通量随时间的沉降损失演化规律.研究结果表明:当电子能量大于0.5 Me V,磁壳参数大于1.6时,甚低频电磁波的共振散射作用显著;随着磁壳参数或电子能量的增大,斜传播甚低频电磁波引起的高阶共振相互作用越来越大;电子全向通量近似随时间呈指数函数形式衰减. 展开更多
关键词 辐射带 波粒共振散射 扩散系数 甚低频电磁波
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黑体辐射公式的多种推导及其在近代物理构建中的意义(Ⅰ) 被引量:1
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作者 曹则贤 《物理》 CAS 北大核心 2021年第11期761-766,共6页
黑体辐射是近代物理史上一只会下金蛋的鹅,是近代物理的摇篮。黑体辐射研究的意义还在于这是唯一一个涉及c,k,h三个普适常数的物理情景。黑体辐射谱抗测量误差的特性带来了辐射标准和绝对温度参照,谱分布公式对模型的不敏感则使得黑体... 黑体辐射是近代物理史上一只会下金蛋的鹅,是近代物理的摇篮。黑体辐射研究的意义还在于这是唯一一个涉及c,k,h三个普适常数的物理情景。黑体辐射谱抗测量误差的特性带来了辐射标准和绝对温度参照,谱分布公式对模型的不敏感则使得黑体辐射成为独特的物理研究母题。黑体辐射谱分布公式,普朗克多角度推导过,德拜推导过,艾伦菲斯特推导过,劳厄推导过,洛伦兹和庞加莱深入讨论过,泡利推导过,玻色推导过,爱因斯坦在20多年的时间里多角度推导过且产出最为丰硕,近代还有从相对论角度的推导,每一个角度的推导都带来了物理学的新内容,这包括量子力学、固体量子论、受激辐射、量子统计、相对论统计,等等。认真回顾黑体辐射研究的历史细节,考察其中的思想概念演化,不啻于体验一次教科书式的学(做)物理之旅,比如也可以尝试给出能量局域分立化的简单新证明。 展开更多
关键词 黑体 黑体辐射 热辐射 空腔辐射 气体运动论 热平衡 不可逆过程 绝对温度 基尔霍夫定律 斯特藩—玻尔兹曼公式 维恩位移公式 维恩谱分布 瑞利—金斯谱分布 能量均分原理 普朗克方程 普朗克函数 普朗克谱分布 振子 能量量子 不连续性 量子力学 作用量量子化 相空间体积量子化 零点能 全同粒子 玻尔兹曼统计 光电效应 受激辐射 玻色—爱因斯坦统计 玻色—爱因斯坦凝聚 费米—狄拉克统计 热力学 电磁学 统计力学 量子 光子 涨落 波粒二象性
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Fast acceleration of “killer” electrons and energetic ions by interplanetary shock stimulated ULF waves in the inner magnetosphere 被引量:11
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作者 ZONG QiuGang WANG YongFu YUAN ChongJing YANG Biao WANG ChenRui ZHANG XiangYun 《Chinese Science Bulletin》 SCIE EI CAS 2011年第12期1188-1201,共14页
Energetic electrons and ions in the Van Allen radiation belt are the number one space weather threat. Understanding how these energetic particles are accelerated within the Van Allen radiation belt is one of the major... Energetic electrons and ions in the Van Allen radiation belt are the number one space weather threat. Understanding how these energetic particles are accelerated within the Van Allen radiation belt is one of the major challenges in space physics. This paper reviews the recent progress on the fast acceleration of "killer" electrons and energetic ions by ultralow frequency (ULF) waves stimulated by the interplanetary shock in the inner magnetosphere. Very low frequency (VLF) wave-particle interaction is considered to be one of the primary electron acceleration mechanisms because electron cyclotron resonances can easily occur in the VLF frequency range. Recently, using four Cluster spacecraft observations, we have found that, after interplanetary shocks impact the Earth’s magnetosphere, energetic electrons in the radiation belt are accelerated almost immediately and continue to accelerate for a few hours. The time scale (a few days) for traditional acceleration mechanisms, based on VLF wave-particle interactions to accelerate electrons to relativistic energies, is too long to explain our observations. Furthermore, we have found that interplanetary shocks or solar wind pressure pulses, with even small dynamic pressure changes, can play a non-negligible role in radiation belt dynamics. Interplanetary shocks interaction with the Earth’s magnetosphere manifests many fundamental space physics phenomena including energetic particle acceleration. The mechanism of fast acceleration of energetic electrons in the radiation belt responding to interplanetary shock impacts consists of three contributing parts: (1) the initial adiabatic acceleration due to strong shock-related magnetic field compression; (2) followed by the drift-resonant acceleration with poloidal ULF waves excited at different L-shells; and (3) particle acceleration due to the quickly damping electric fields associated with ULF waves. Particles end up with a net acceleration because they gain more energy in the first half of this cycle than they lose in the second. The results reported in this paper cast a new light on understanding the acceleration of energetic particles in the Earth’s Van Allen radiation belt. The results of this study can likewise be applied to interplanetary shock interaction with other planets such as Mercury, Jupiter, Saturn, Uranus and Neptune, and other astrophysical objects with magnetic fields. 展开更多
关键词 行星际激波 高能离子 高能电子 地球磁层 ULF 激波加速 粒子相互作用 电子回旋共振
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