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Dark Galaxies, Sun-Earth-Moon Interaction, Tunguska Event—Explained by WUM
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作者 Vladimir S. Netchitailo 《Journal of High Energy Physics, Gravitation and Cosmology》 CAS 2024年第2期836-853,共18页
Great experimental results and observations achieved by Astronomy in the last decades revealed new unexplainable phenomena. Astronomers have conclusive new evidence that a recently discovered “dark galaxy” is, in fa... Great experimental results and observations achieved by Astronomy in the last decades revealed new unexplainable phenomena. Astronomers have conclusive new evidence that a recently discovered “dark galaxy” is, in fact, an object the size of a galaxy, made entirely of dark matter. They found that the speed of the Earth’s rotation varies randomly each day. 115 years ago, the Tunguska Event was observed, and astronomers still do not have an explanation of It. Main results of the present article are: 1) Dark galaxies explained by the spinning of their Dark Matter Cores with the surface speed at equator less than the escape velocity. Their Rotational Fission is not happening. Extrasolar systems do not emerge;2) 21-cm Emission explained by the self-annihilation of Dark Matter particles XIONs (5.3 μeV);3) Sun-Earth-Moon Interaction explained by the influence of the Sun’s and the Moon’s magnetic field on the electrical currents of the charged Geomagma (the 660-km layer), and, as a result, the Earth’s daylength varies;4) Tunguska Event explained by a huge atmospheric explosion of the Superbolide, which was a stable Dark Matter Bubble before entering the Earth’s atmosphere. 展开更多
关键词 World-Universe Model Dark Stars Dark Galaxies 21-cm emission Formation of Macrostructures Sun-Earth-moon Interaction Tunguska Event Dark Matter
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NITROGEN DETERMINATION IN THE SURFACE OF NITRIDED STEEL USING PROTON INDUCED GAMMA-RAY EMISSION ANALYSIS
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作者 廖常庚 汪永强 +2 位作者 项金钟 马志辉 郑志豪 《Chinese Science Bulletin》 SCIE EI CAS 1989年第4期279-283,共5页
Ⅰ. INTRODUCTIONIt has been established for some time that introduction of nitrogen in the surface and near surface regions of metal alloys can make important modifications in surface properties of the alloys such as ... Ⅰ. INTRODUCTIONIt has been established for some time that introduction of nitrogen in the surface and near surface regions of metal alloys can make important modifications in surface properties of the alloys such as hardness, wear and friction, corrosion resistance and fatigue time. Proton induced gamma-ray emission (PIGE) analysis provides a useful method for direct determination of nitrogen concentration in the surface of nitrided samples and also for its quality test and the investigation of new nitriding technology.The aims of the present work are to study the optimum conditions of 展开更多
关键词 PROTON INDUCED gamma-ray emission NITROGEN CONCENTRATION DEPTH profile.
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嫦娥一号宇生伽马射线能谱分析 被引量:2
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作者 张婧瑶 王南萍 《原子能科学技术》 EI CAS CSCD 北大核心 2014年第S1期9-13,共5页
介绍了一种通过宇生伽马射线分析月表部分元素含量的方法。我国嫦娥一号卫星携带的伽马射线能谱仪(CE1-GRS)探测的伽马射线能谱中,既包含月表天然放射性元素(K、U、Th等)放出的伽马射线,也包含银河宇宙射线(GCR)与月表物质(Fe、Si、O等... 介绍了一种通过宇生伽马射线分析月表部分元素含量的方法。我国嫦娥一号卫星携带的伽马射线能谱仪(CE1-GRS)探测的伽马射线能谱中,既包含月表天然放射性元素(K、U、Th等)放出的伽马射线,也包含银河宇宙射线(GCR)与月表物质(Fe、Si、O等)发生簇射反应过程中产生的伽马射线。根据已知GCR的强度和能量分布,使用蒙特卡罗方法模拟,计算出GCR与月表物质反应产生的伽马射线特征峰及面积,并与CE1-GRS测量谱线相比较,建立了几种元素测量谱线与其月表含量的关系,该方法将可用于月表非天然放射性元素平均含量的计算。 展开更多
关键词 月球探测 CE1-GRS 伽马能谱 月表伽马射线
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基于Clementine热红外数据的Apollo17登月点区域氧化钙含量反演 被引量:2
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作者 刘道飞 陈圣波 路鹏 《地球学报》 EI CAS CSCD 北大核心 2015年第2期245-249,共5页
为了研究利用Clementine热红外数据反演月球表面岩石的氧化钙(Ca O)含量,论文选取了两景覆盖Apollo17登月点的Clementine热红外影像,将其覆盖的区域选为研究区。利用月球表面温度物理模型模拟月表温度,结合普朗克函数,完成发射率反演。... 为了研究利用Clementine热红外数据反演月球表面岩石的氧化钙(Ca O)含量,论文选取了两景覆盖Apollo17登月点的Clementine热红外影像,将其覆盖的区域选为研究区。利用月球表面温度物理模型模拟月表温度,结合普朗克函数,完成发射率反演。在此基础上,对LPI中35个除Apollo17登月计划外所采集的样品Ca O含量与其热红外发射率特征做回归统计分析,发现存在很好的线性关系(R2=0.661)。由此,基于Clementine热红外发射率实现了研究区Ca O含量反演。通过利用LPI Apollo17月岩(壤)样品实际Ca O含量分析数据对反演结果进行精度评价,发现8组反演值与实际值的相对误差最小为1.77%,最大为9.29%,均方根误差为0.767。研究结果表明,使用发射率进行Ca O含量反演方法可行,为利用Clementine热红外数据对月表矿物成分含量定量反演提供一种新的思路。 展开更多
关键词 月球 CLEMENTINE 热红外 Apollo17 发射率 氧化钙
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高温熔盐体系惰性阳极与月壤电解制氧技术 被引量:2
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作者 寇明银 王明涌 焦树强 《工程科学学报》 EI CSCD 北大核心 2021年第12期1618-1629,共12页
目前,熔盐电化学冶金普遍采用炭素阳极,阳极CO_(2)产物是重要的碳排放源.若在高温熔盐体系中使用惰性析氧阳极,则可实现熔盐电解过程低碳排放.因此,开发适用于熔盐电解体系的惰性阳极至关重要,也是近年来国内外研究热点.本文首先综述了... 目前,熔盐电化学冶金普遍采用炭素阳极,阳极CO_(2)产物是重要的碳排放源.若在高温熔盐体系中使用惰性析氧阳极,则可实现熔盐电解过程低碳排放.因此,开发适用于熔盐电解体系的惰性阳极至关重要,也是近年来国内外研究热点.本文首先综述了各种高温熔盐体系惰性阳极的研究进展,所涉及熔盐体系包括:铝电解氟化物盐、CaCl_(2)熔盐、碳酸盐和熔融氧化物等.另外,近年来月球开发利用受到广泛关注,太阳能驱动的月壤原位熔盐电化学制氧,将是支撑人类未来月面生存氧气需求的重要方法之一,故惰性析氧阳极不可或缺.因此,本文也简要综述了基于惰性阳极的月壤电解制氧技术. 展开更多
关键词 碳减排 高温熔盐 惰性阳极 熔盐电解 月壤制氧
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One-Dimensional Electric Field Structure of an Outer Gap Accelerator
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作者 陈世波 张力 《Chinese Physics Letters》 SCIE CAS CSCD 2006年第10期2881-2884,共4页
We re-study the one-dimensional electric field structure of an outer gap accelerator by considering the physical limit of trans-field height. Inside the outer gap, the charge depletion creates a large electric field a... We re-study the one-dimensional electric field structure of an outer gap accelerator by considering the physical limit of trans-field height. Inside the outer gap, the charge depletion creates a large electric field along the magnetic field lines. Electrons and/or positrons are accelerated to ultra-relativistic energies by this longitudinal electric field, and then radiate γ-ray photons by curvature radiation. The collision of these γ-rays and ambient x-ray photons further produce radiating particles, resulting in a stationary gap. We solve the structure of this longitudinal electric field together with the distributions of electrons and positrons and γ-ray photons for an aligned rotator. Our results indicate that the outer gap can extend to the light cylinder using reasonable parameters. 展开更多
关键词 gamma-ray emission RAPIDLY SPINNING PULSARS CURVATURE RADIATION SPECTRA MAGNETOSPHERE MODEL
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AGN Singularities and Jets Modelled with the Superstar Scenario
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作者 Ding-Yu Chung 《International Journal of Astronomy and Astrophysics》 2019年第2期142-153,共12页
In this paper we present solutions with the superstar scenario for the problems of singularity and the relativistic jet in AGN (Active Galactic Nuclei) based on supermassive black hole with singularity. The five-zone ... In this paper we present solutions with the superstar scenario for the problems of singularity and the relativistic jet in AGN (Active Galactic Nuclei) based on supermassive black hole with singularity. The five-zone structure of superstar from inside to outside consists of the Singularity-Free Superstar Core (SC), the short-range repulsive super force field (SFF) near the event horizon, the superstar lepton sphere (SLS) containing infalling leptons (electron-positron pairs), the superstar ergosphere (SE), and the superstar accretion disk (SAD). As in the Meissner effect in superconductor, the short-range SFF repulses leptons in the SLS preventing singularity, while infalling leptons from the SAD and the SE continue to enter the SLS through the strong gravity of the SC. When the density at the bottom of the SLS reaches the critical density, leptons fall into the SC with the corresponding size increase of the SC to prevent singularity. Without further infalling leptons, the short-range repulsive force from the SFF disintegrates the SLS into the SLS plasma fragments (electron-positron pair plasma), detaching from the SC. Some SLS plasma fragments in the SAD generate the broad relativistic SAD jet, and some SLS plasma fragments in the SE generate the coincident narrow relativistic SE jet. In this two-jet model (the origin of the spine-sheath jet structure), protected by the SAD jet, the fast and narrow SE jet inside the slow and broad SAD jet generates the VHE (very high energy ≥ 100 GeV) Synchrotron Self Compton (SSC) gamma-ray emission without the attenuation by the photons in the BLR (broad line region) of flat spectrum radio quasar (FSRQ). In conclusion, AGN based on supermassive superstar provide the solutions for singularity, VHE gamma-ray emissions in FSRQs and FR1 type radio galaxies, AGN jet structure, and AGN jet type. 展开更多
关键词 ANG RELATIVISTIC Jet SUPERSTAR Supermassive SINGULARITY Black Hole Super Force Field Very High Energy gamma-ray emission
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Recent observations and research progresses of terrestrial gamma-ray flashes during thunderstorms
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作者 Fanchao LYU Yijun ZHANG +5 位作者 Gaopeng LU Baoyou ZHU Hongbo ZHANG Wei XU Shaolin XIONG Weitao LYU 《Science China Earth Sciences》 SCIE EI CAS CSCD 2023年第3期435-455,共21页
Terrestrial gamma-ray flashes(TGFs)are high-energy emissions in thunderstorms that were discovered first by satellite-based and then by ground-based gamma-ray detectors with photon energy up to tens of Me V.TGFs are a... Terrestrial gamma-ray flashes(TGFs)are high-energy emissions in thunderstorms that were discovered first by satellite-based and then by ground-based gamma-ray detectors with photon energy up to tens of Me V.TGFs are a natural highenergy phenomenon associated with lightning discharges that frequently occur during thunderstorms.However,their production mechanisms and associated processes are still unclear.TGF studies have already been a research spotlight in the atmospheric electricity and high-energy atmosphere research areas.In this paper,we review recent research progresses on TGF studies in the past decade,including TGF detection,the relationship between TGFs and lightning processes,and thunderstorm activities.Several unsolved important scientific questions are discussed.Results suggest that upward TGFs observed by satellite-based detectors are closely connected with the development of in-cloud upward negative leaders.They are usually generated in milliseconds of the initiation of upward negative leaders and may produce a kind of distinct radio emissions because of the generation and propagation of huge amounts of high-energy electrons.By contrast,its counterpart,i.e.,downward TGFs observed by ground-based gamma-ray detectors,is associated with different types of lightning processes,such as downward negative or upward positive leaders,the initial continuing current stage of rocket-triggered lightning flashes return stroke processes.Because of limited observations,how these downward TGFs are generated is still unclear.Benefiting from the development of state-of-the-art instruments with high temporal and spatial resolutions,new insights into the processes and mechanisms of TGFs will be achieved with coordinated observations from satellite-based and ground-based measurements. 展开更多
关键词 Terrestrial gamma-ray flashes(TGFs) LIGHTNING THUNDERSTORM High-energy emissions Radio emission detection
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On the detectability of Galactic dark matter annihilation into monochromatic gamma-rays
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作者 唐志成 袁强 +1 位作者 毕效军 陈国明 《Chinese Physics C》 SCIE CAS CSCD 2011年第8期725-734,共10页
Monochromatic y-rays are thought to be the smoking gun signal for identifying dark matter annihilation. However, the flux of monochromatic y-rays is usually suppressed by virtual quantum effects since dark matter shou... Monochromatic y-rays are thought to be the smoking gun signal for identifying dark matter annihilation. However, the flux of monochromatic y-rays is usually suppressed by virtual quantum effects since dark matter should be neutral and does not couple with y-rays directly. In this work, we study the detection strategy of the monochromatic y-rays in a future space-based detector. The flux of monochromatic y-rays between 50 GeV and several TeV is calculated by assuming the supersymmetric neutralino as a typical dark matter candidate. The detection both by focusing on the Galactic center and in a scan mode that detects y-rays from the whole Galactic halo are compared. The detector performance for the purpose of monochromatic y-ray detection, with different energy and angular resolution, field of view, and background rejection efficiencies, is carefully studied with both analytical and fast Monte-Carlo methods. 展开更多
关键词 dark matter line emission gamma-ray DETECTABILITY
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