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Superposing the Magnetic Spiral Structure of the Milky Way, on the Stellar Spiral Arms—Matching the Unique Galactic Magnetic Field Reversal Zone with Two Galactic Spiral Arm Segments 被引量:1
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作者 Jacques P. Vallée 《International Journal of Astronomy and Astrophysics》 2022年第4期281-300,共20页
To pinpoint the peak location of the synchrotron total intensity emission in a spiral arm, we use a map of the spiralarm locations (from the observed arm tangent). Thus in a typical spiral arm in Galactic Quadrant I, ... To pinpoint the peak location of the synchrotron total intensity emission in a spiral arm, we use a map of the spiralarm locations (from the observed arm tangent). Thus in a typical spiral arm in Galactic Quadrant I, we find the peak of the synchrotron radiation to be located about 220 ± 40 pc away from the inner arm edge (hot dust lane) inside the spiral arm. While most of the galactic disk has a clockwise large-scale magnetic field, we make a statistical analysis to delimitate more precisely the smaller reverse annulus with a counterclockwise galactic magnetic field. We find an annulus width of 2.1 ± 0.3 kpc (measured along the Galactic radius), located from 5.5 to 7.6 kpc from the Galactic Center). The annulus does not overlay with a single spiral arm—it encompasses segments of two different spiral arms. Using a recent delineation of the position of spiral arms, the field-reversed annulus is seen to encompass the Crux-Centaurus arm (in Galactic Quadrant IV) and the Sagittarius arm (in Galactic Quadrant I). Thus the full Sagittarius-Carina arm is composed of: 1) a Sagittarius arm (in Galactic quadrant I) with a counterclockwise magnetic field, and 2) a Carina arm (in Galactic Quadrant IV) with a clockwise magnetic field. Also the full Scutum-Crux-Centaurus arm is composed of: 1) a Scutum arm (in Galactic Quadrant I) with a clockwise magnetic field, and 2) a Crux-Centaurus arm (in Galactic Quadrant IV) with a counterclockwise magnetic field. Arm segments do not all have the same magnetic field direction. For completeness, we display 6 known magnetised advancing supershells around the Sun (within 400 pc), pushing out the interstellar magnetic field. 展开更多
关键词 ASTROPHYSICS Galaxy Milky Way spiral arms SYMMETRIES
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A Method of Obtaining the Pitch Angle of Spiral Arms and the Inclination of Galactic Discs
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作者 Jun Ma (National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012) E-mail:majun@vega.bac.pku.edu.cn 《Chinese Journal of Astronomy and Astrophysics》 CSCD 北大核心 2001年第5期395-405,共11页
We investigate the mathematical form, the symmetry of spiral structure and the projected images of galactic discs. The measured pitch angles of spiral arms and inclination angles of galactic discs for 60 spiral galaxi... We investigate the mathematical form, the symmetry of spiral structure and the projected images of galactic discs. The measured pitch angles of spiral arms and inclination angles of galactic discs for 60 spiral galaxies are presented. The global spiral structure is emphasized in the study. It is found that, except for small-scale distortions, the spiral arms of those galaxies that were classified as AC 12 in the arm classification system of Elmegreen & Elmegreen, can be represented by the logarithmic spiral form. 展开更多
关键词 galaxies: spiral galaxies - galaxies: spiral arm disc: inclination
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Kinematic Structure of the Milky Way Galaxy, Near the Spiral Arm Tangents
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作者 Jacques P. Vallée 《International Journal of Astronomy and Astrophysics》 2022年第4期382-392,共11页
We compare the observed radial velocity of different arm tracers, taken near the tangent to a spiral arm. A slight difference is predicted by the density wave theory, given the shock predicted at the entrance to the i... We compare the observed radial velocity of different arm tracers, taken near the tangent to a spiral arm. A slight difference is predicted by the density wave theory, given the shock predicted at the entrance to the inner spiral arm. In many of these spiral arms, the observed velocity offset confirms the prediction of the density wave theory (with a separation between the maser velocity and the CO gas peak velocity, of about 20 km/s)—when the observed offset is bigger than the error estimates. 展开更多
关键词 ASTROPHYSICS GALAXY Milky Way spiral arms SYMMETRIES
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Particle Paths of Lagrangian Velocity Distribution Simulating the Spiral Arms of Galaxy M51 被引量:1
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作者 Georgios H.Vatistas 《Journal of Thermal Science》 SCIE EI CAS CSCD 2008年第1期61-63,共3页
Galaxies are huge families of stars held together by their own gravities. The system M51 is a spiral galaxy. It possesses billions of stars. The range of the spiral arms extends hundred thousand light years. The prese... Galaxies are huge families of stars held together by their own gravities. The system M51 is a spiral galaxy. It possesses billions of stars. The range of the spiral arms extends hundred thousand light years. The present study is in an attempt in using the particle paths of the Lagrangian flow field to simulate the spiral arms of Galaxy M51. The Lagrangian flow field is introduced. The initial locations of fluid particles in the space between two concen- tric cylinders are ftrst specified. Then a linear velocity distribution of the fluid particles is used with different an- gle rotations of the particles to obtain the particle paths in the Lagrangian diagram. For simulating the spiral arms of Galaxy M51, the Lagrangian M51 diagram is developed. The particle paths of the Lagrangian M51 diagram agree quite well with the spiral arms of Galaxy M51. 展开更多
关键词 Lagrangian flow field Particle path Dimensionless normalization spiral arms Galaxy M51
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Arm Tangents and the Spiral Structure of the Milky Way—The Age Gradient 被引量:2
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作者 Jacques P. Vallée 《International Journal of Astronomy and Astrophysics》 2021年第4期445-457,共13页
From the Sun, a look at the edge of each spiral arm in our Milky Way (seen tangentially, along the line of sight) can yield numerous insights. Using different arm tracers (dust, masers, synchrotron emission, CO gas, o... From the Sun, a look at the edge of each spiral arm in our Milky Way (seen tangentially, along the line of sight) can yield numerous insights. Using different arm tracers (dust, masers, synchrotron emission, CO gas, open star clusters), we observe here for the first time an age gradient (about 12 ± 2 Myrs/kpc), much as predicted by the density wave theory. This implies that the arm tracers are leaving the dust lane at a relative speed of about 81 ± 10 km/s. We then compare with recent optical data obtained from the Gaia satellite, pertaining to the spiral arms. 展开更多
关键词 ASTROPHYSICS GALAXY Milky Way spiral arms
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Motion Law of Graviton in Three-Dimensional Space and Its Influence on Star Distribution of Spiral Galaxy 被引量:1
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作者 Pingan Luo 《Journal of Modern Physics》 2014年第17期1910-1930,共21页
According to some fundamental hypotheses compatible with microphysics theory in allusion to property of graviton shot by the spiral galaxy, we set up a motion trace equation of graviton in the three-dimensional space,... According to some fundamental hypotheses compatible with microphysics theory in allusion to property of graviton shot by the spiral galaxy, we set up a motion trace equation of graviton in the three-dimensional space, concluding method for measuring the velocity of graviton. This theory reveals formation mechanism of symmetric rotating arm image of the spiral galaxy. The rotating arm image conforms to Archimedes spiral. Under the condition of using dynamic constraints, the image that astrolabe is in thin-disk structure is naturally obtained. And then, we also deduce the law that astrolabe thickness h is inversely proportional to the square root of the distance rxy between astrolabe and galaxy center, according with actual crossrange galaxy observation image excellently. This article, by utilizing several typical galaxy observation images with completely different appearances and shapes, verifies the motion trace law of graviton in three-dimensional space. And the theoretical simulation data meet observation image data very well. As per the discovery in the simulation of three-dimensional theoretical model, changes of parameters in theoretical model will exert a great influence on the shape of galaxy. This theory owns exclusively important meaning, not only to astrophysics, but also to reconstruction and development of relativity theory and the whole basic physics theory, as well as breaking through the current dilemma in studying graviton property. 展开更多
关键词 Graviton The Velocity of Graviton MOTION TRACE spiral GALAXY M51 SYMMETRIC Double spiral arm Thin DISK
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多臂螺旋传声器阵列的优化设计
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作者 任豪杰 张二亮 +1 位作者 朱松 曹雪林 《传感器与微系统》 CSCD 北大核心 2024年第7期67-71,共5页
针对基于经验或者数学模型的阵列设计不能充分挖掘传声器阵列声学定位潜力的问题,提出了一种多臂螺旋阵列的通用设计模型,以波束的主瓣宽度(MLW)和最大旁瓣水平(MSL)为评价指标,采用非支配排序遗传进化算法对模型参数进行迭代优化,获得... 针对基于经验或者数学模型的阵列设计不能充分挖掘传声器阵列声学定位潜力的问题,提出了一种多臂螺旋阵列的通用设计模型,以波束的主瓣宽度(MLW)和最大旁瓣水平(MSL)为评价指标,采用非支配排序遗传进化算法对模型参数进行迭代优化,获得传声器阵列构型的非支配解集。针对56传声器多臂螺旋阵列,首先以传声器极径为设计变量,随后开展了传声器极径与螺旋角协同设计。结果表明,所设计的传声器阵列在宽频范围内具有稳定的MSL,考虑螺旋角的协同设计创新了多臂螺旋阵列的布局形式,进一步降低波束的MLW和MSL。最后,基于邻近双声源定位算例,通过与常规对数多臂螺旋阵列和Underbrink螺旋阵列对比,验证了所设计传声器阵列具有较高的空间分辨和空间干扰抑制能力。 展开更多
关键词 多臂螺旋传声器阵列 优化设计 多目标优化 波束形成
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交叉耦合馈电的小型化八臂缝隙螺旋天线
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作者 傅立炜 袁家德 牟泓舟 《微波学报》 CSCD 北大核心 2024年第5期61-65,共5页
研究了一种应用于卫星导航终端的小型化交叉耦合馈电八臂缝隙螺旋天线。八条缝隙螺旋臂作为天线的辐射单元,蚀刻在FR4介质基板构成的方形柱状结构的外表面。馈电网络为上、下相互正交四分之三圆环的交叉偶极子微带线结构,延伸至了外表... 研究了一种应用于卫星导航终端的小型化交叉耦合馈电八臂缝隙螺旋天线。八条缝隙螺旋臂作为天线的辐射单元,蚀刻在FR4介质基板构成的方形柱状结构的外表面。馈电网络为上、下相互正交四分之三圆环的交叉偶极子微带线结构,延伸至了外表面且实现了交叉耦合馈电。天线尺寸为0.082λ0×0.082λ0×0.130λ0(λ0为中心频率1.561 GHz对应的自由空间波长),实测结果显示,|S11|≤-10 dB的阻抗带宽为1.554 GHz~1.591 GHz,3 dB轴比带宽为1.535 GHz~1.594 GHz。在北斗卫星导航系统B1频段中心频率(1.561 GHz)和全球定位系统L1频段中心频率(1.575 GHz)处的增益分别达到了2.56 dBi和2.75 dBi。该天线采用八臂缝隙螺旋和交叉偶极子臂耦合馈电相结合的结构,实现了较好的圆极化性能,同时具备宽频带和小型化的特点。 展开更多
关键词 耦合馈电 交叉偶极子 八臂缝隙螺旋天线 卫星导航终端 圆极化
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Life Origin in the Milky Way Galaxy: III. Spatial Distribution of Overheated Stars in the Solar Neighborhood
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作者 Alexander N. Safronov 《Journal of High Energy Physics, Gravitation and Cosmology》 CAS 2024年第2期693-709,共17页
A concept of ensemble averaged stellar reactors is developed to study the dynamics of processes occurring in stars, allocated in the ~200 pc solar neighborhood. According to the effective temperature value, four stell... A concept of ensemble averaged stellar reactors is developed to study the dynamics of processes occurring in stars, allocated in the ~200 pc solar neighborhood. According to the effective temperature value, four stellar classes are identified, for which the correlation coefficients and standard deviation are counted. The theory of the buoyancy terrestial elements is generalized to stellar systems. It was suggested that stars are over-heated due to the shift parameters of the nuclear processes occurring inside the stars, which leads to the synthesis of transuranium elements until the achievement of a critical nuclear mass and star explosion. The heavy transuranium elements sink downward and are concentrated in the stellar depth layers. The physical explanation of the existence of the critical Chandrasekhar star limit has been offered. Based on the spatial analysis of overheated stars, it was suggested that the withdrawal of the stellar reactor from the equilibrium state is a consequence of extragalactic compression inside the galaxy arm due to the arm spirality (not to be confused with the spirality of the galaxy itself). 展开更多
关键词 Stellar Nucleogenesis Ensemble-Averaged Stellar Reactor Overheated Stars Chandrasekhar Stellar Limit arm spirality
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介质阻挡流光放电中的螺旋波与靶波 被引量:11
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作者 刘富成 董丽芳 +1 位作者 贺亚峰 尹增谦 《河北大学学报(自然科学版)》 CAS 2004年第3期251-254,共4页
采用双水电极实验装置,对大气压氩气介质阻挡放电中的靶波与螺旋波斑图进行了观察测量.实验发现靶波与螺旋波可以互相转变,且有2种不同的转变路径:靶波→单臂螺旋波→靶波→单臂螺旋波;靶波→单臂螺旋波→双臂螺旋波→靶波.
关键词 靶波 单臂螺旋波 双臂螺旋波 转变路径
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一种高效率圆极化背腔天线阵的设计 被引量:2
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作者 宋长宏 吴群 +1 位作者 张文静 路志勇 《电波科学学报》 EI CSCD 北大核心 2014年第1期129-134,共6页
设计了一种新型单臂螺旋边馈阶梯喇叭圆极化背腔天线,天线单元由阶梯喇叭、单臂螺旋及圆形背腔组成.单臂螺旋采用准空气同轴线激励,给出了天线单元的轴比、驻波、方向图宽频带特性.提出单元旋转反相馈电方法改善了天线子阵轴比和极化隔... 设计了一种新型单臂螺旋边馈阶梯喇叭圆极化背腔天线,天线单元由阶梯喇叭、单臂螺旋及圆形背腔组成.单臂螺旋采用准空气同轴线激励,给出了天线单元的轴比、驻波、方向图宽频带特性.提出单元旋转反相馈电方法改善了天线子阵轴比和极化隔离,同时解决了馈电空间狭小的难题.对阵列进行了加工测试,测试与仿真结果吻合.结果显示,天线增益、驻波带宽、轴比带宽和方向图性能优良,此种天线具有很好的工程应用前景. 展开更多
关键词 单臂螺旋 阶梯喇叭 圆极化 高效率
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飞机起落架噪声测量平面阵列设计仿真研究 被引量:3
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作者 陈涛 侯宏 辛渊博 《计算机仿真》 CSCD 北大核心 2011年第9期83-85,113,共4页
研究飞机消除噪声的优化问题,针对飞机机体噪声对环境的污染,需要对飞机起落架(机体主要噪声源)的噪声特性进行测量分析,正确地认识起落架噪声的产生机理,为设计人员降低机体噪声提供数据和理论支持。为了将起落架噪声从飞机总体噪声中... 研究飞机消除噪声的优化问题,针对飞机机体噪声对环境的污染,需要对飞机起落架(机体主要噪声源)的噪声特性进行测量分析,正确地认识起落架噪声的产生机理,为设计人员降低机体噪声提供数据和理论支持。为了将起落架噪声从飞机总体噪声中分离出来,研究平面阵的设计,提出了多臂螺旋阵的设计方案。对比了十字阵、均匀圆阵、多臂螺旋阵等的常规波束空间谱估计图,发现在传感器个数有限的条件下,多臂螺旋阵比十字阵和均匀圆阵能获得更小的主瓣宽度和更好的旁瓣抑制能力。根据对国产飞机ARJ21过顶飞行进行起落架噪声测量的要求,对多臂螺旋阵的起始半径、最大半径对主瓣宽度和旁瓣抑制水平的影响进行了仿真,找到了在传声器个数固定的情况下的最佳的多臂螺旋阵的设计方案。 展开更多
关键词 主瓣宽度 多臂螺旋阵 起落架噪声
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瓦斯抽采钻孔螺旋式水力机械扩孔装置及其应用 被引量:5
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作者 徐超 孙浩石 +3 位作者 秦亮亮 闫志铭 郭超飞 杨港 《西安科技大学学报》 CAS 北大核心 2021年第4期640-648,共9页
水力机械扩孔增透技术是提高煤层瓦斯抽采效果、预防煤层瓦斯突出的重要方法之一。目前水力机械扩孔装置多采用直角式刀臂结构,但直角式刀臂在应用过程中存在着塌孔严重、排渣不畅、扩孔初期刀臂遇阻展开不畅以及水压动力分配不均等缺陷... 水力机械扩孔增透技术是提高煤层瓦斯抽采效果、预防煤层瓦斯突出的重要方法之一。目前水力机械扩孔装置多采用直角式刀臂结构,但直角式刀臂在应用过程中存在着塌孔严重、排渣不畅、扩孔初期刀臂遇阻展开不畅以及水压动力分配不均等缺陷,严重影响着煤层扩孔的施工效果。基于此,研发一种瓦斯抽采钻孔螺旋式水力机械扩孔装置,将刀臂结构由传统的直角式改变为螺旋式,设计内部动力驱动装置,并提供一种高低压水切换装置以控制各管路开闭,进而完善煤层扩孔工艺流程。所设计的螺旋式水力机械扩孔装置在阳煤集团平舒煤矿15211工作面进行试点应用,结果表明:螺旋式刀臂较直角式刀臂拥有更好的切削煤体能力,扩孔装置卡刀次数明显减少,扩孔总长度提升10.59%,成孔率提高12.5%,并将扩孔总施工周期缩短1 d。证明螺旋式水力机械扩孔装置结构设计的合理性与优越性,为煤矿井下扩孔设备的优化改进提供了方向。 展开更多
关键词 松软煤层 瓦斯抽采 螺旋式刀臂 扩孔装置 结构设计
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倾斜波束非对称SAARS微带天线设计 被引量:4
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作者 李思佳 曹祥玉 +2 位作者 高军 郑秋容 杨欢欢 《西安电子科技大学学报》 EI CAS CSCD 北大核心 2014年第1期164-169,共6页
为了实现圆极化天线的倾斜波束,在单臂阿基米德螺旋(Single-Arm ARchimedean Spiral,SAARS)天线的基础上,联合柱状螺旋天线的非对称结构,设计出了一款波束倾角为30°的等圈非对称圆极化天线.通过对螺旋臂参数和馈电连接线的优选,拓... 为了实现圆极化天线的倾斜波束,在单臂阿基米德螺旋(Single-Arm ARchimedean Spiral,SAARS)天线的基础上,联合柱状螺旋天线的非对称结构,设计出了一款波束倾角为30°的等圈非对称圆极化天线.通过对螺旋臂参数和馈电连接线的优选,拓展了天线的带宽,优化了天线的辐射性能.在垂直孔径同轴馈电方式的激励下,同时考虑电压驻波比小于2、轴比小于3dB和30°倾斜波束的条件,天线工作的相对带宽约达16.7%.仿真和实测结果吻合较好,表明所设计的天线不仅具有良好的带宽、较高的增益,同时实现了圆极化波束倾斜. 展开更多
关键词 微带天线 圆极化 倾斜波束 单臂阿基米德螺旋线 非对称结构
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ARJ客机过顶飞行过程噪声的实验研究 被引量:1
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作者 陈涛 侯宏 +1 位作者 陈志菲 赵江楠 《计量学报》 CSCD 北大核心 2012年第5期437-440,共4页
对ARJ客机过顶的噪声源进行了现场实验分析。为了将飞机不同噪声源分开,利用了阵列信号处理技术,设计了多臂螺旋阵。实验发现:ARJ飞机的噪声源主要分布在发动机、起落架、襟翼、尾翼后部等位置,不同频率下,主要噪声源的组成不同,... 对ARJ客机过顶的噪声源进行了现场实验分析。为了将飞机不同噪声源分开,利用了阵列信号处理技术,设计了多臂螺旋阵。实验发现:ARJ飞机的噪声源主要分布在发动机、起落架、襟翼、尾翼后部等位置,不同频率下,主要噪声源的组成不同,为飞机降噪工作提供了支持。 展开更多
关键词 计量学 飞机噪声 阵列处理技术 多臂螺旋阵
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一种用于超高频电磁信号检测的单臂阿基米德螺旋天线的设计 被引量:1
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作者 喇元 吴俊锋 欧小波 《电测与仪表》 北大核心 2014年第5期61-66,共6页
研究了一种50Ω同轴电缆直接馈电的单臂阿基米德螺旋天线,通过优化仿真设计了天线各项硬件参数,实现了其在UHF(超高频)段的工作。通过锥形金属片过渡馈电的方式保证了天线结构的稳定性,克服了单臂阿基米德螺旋天线偏心馈电带来的不良影... 研究了一种50Ω同轴电缆直接馈电的单臂阿基米德螺旋天线,通过优化仿真设计了天线各项硬件参数,实现了其在UHF(超高频)段的工作。通过锥形金属片过渡馈电的方式保证了天线结构的稳定性,克服了单臂阿基米德螺旋天线偏心馈电带来的不良影响。通过改进天线的终端结构,节约了天线制作材料,提升了天线的整体性能。通过仿真分析研究了天线介质材料、馈电圆锥角、天线占空比等对天线性能的影响,并进行了优化设计。结果表明,设计的天线结构简单无需馈电巴伦,其工作频带为:1.15GHz^2.4GHz,具有良好的圆极化特性,在工作频带范围内天线最大辐射方向具有5dB以上的增益,基本满足超高频电磁信号的检测要求。 展开更多
关键词 单臂阿基米德螺旋 超高频 无巴伦 圆极化 优化仿真
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一种矿用定向天线设计 被引量:1
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作者 王婷婷 徐钊 《工矿自动化》 北大核心 2016年第2期55-57,共3页
设计了一款适用于巷道类狭长受限空间的双臂平面螺旋天线。该天线由4条等角螺旋线构造的2个对称的螺悬臂组成。与传统的全向天线相比,该天线辐射的定向波束可减少无线电波在巷道壁上的反射损耗,圆极化特性可有效减弱巷道内多径效应的影... 设计了一款适用于巷道类狭长受限空间的双臂平面螺旋天线。该天线由4条等角螺旋线构造的2个对称的螺悬臂组成。与传统的全向天线相比,该天线辐射的定向波束可减少无线电波在巷道壁上的反射损耗,圆极化特性可有效减弱巷道内多径效应的影响,双向辐射特性可提高辐射效率。仿真结果表明,工作在2.4GHz频段时,5圈双臂平面螺旋天线的3dB半功率波瓣宽度大于60°,增益大于4dB;10圈双臂平面螺旋天线的3dB半功率波瓣宽度为120°,增益大于6dB。 展开更多
关键词 双臂平面螺旋天线 圆极化 有向辐射 抗多径
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介质阻挡放电中螺旋波斑图的臂数变化
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作者 刘书华 董丽芳 +3 位作者 王红芳 刘微粒 郝雅娟 冉俊霞 《河北大学学报(自然科学版)》 CAS 北大核心 2007年第4期357-360,共4页
本工作利用介质阻挡放电装置,观察到单臂螺旋波、多臂螺旋波与靶波,发现在参数不变的情况下,不同臂数的螺旋波斑图可以相互转化.利用唯象模型模拟了不同臂数螺旋波的演变过程,结果显示:拓扑缺陷(断层)向螺旋波中心移动时,会引起螺旋波... 本工作利用介质阻挡放电装置,观察到单臂螺旋波、多臂螺旋波与靶波,发现在参数不变的情况下,不同臂数的螺旋波斑图可以相互转化.利用唯象模型模拟了不同臂数螺旋波的演变过程,结果显示:拓扑缺陷(断层)向螺旋波中心移动时,会引起螺旋波臂数的改变,若断层与螺旋波拓扑荷同号,螺旋波臂数增加,若断层与螺旋波拓扑荷反号,螺旋波臂数将减少. 展开更多
关键词 介质阻挡放电 斑图动力学 多臂螺旋波 断层
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Cosmic Contributions to the Deposition of Petroleum Source Rocks: Review and Analysis 被引量:1
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作者 Heinz-Jürgen Brink 《International Journal of Geosciences》 2023年第11期1123-1145,共23页
The development of globally distributed Phanerozoic petroleum source rocks is concentrated on time intervals, which correlate convincingly with climatic driven glaciation epochs of Earth’s history, repeated every 150... The development of globally distributed Phanerozoic petroleum source rocks is concentrated on time intervals, which correlate convincingly with climatic driven glaciation epochs of Earth’s history, repeated every 150 million years, and during sea level high stands and maxima of global magmatism with a period of 300 million years. The 150 million year periodicity appears to be related to the path of the solar system through the spiral arms of the Milky Way and the 300 million year periodicity to changes of the spiral system. The spiral arms are preferred birth places of new stars, of which the larger ones have only smaller lifespans. Their preliminary deaths ended with explosions and selectively with the development of so-called white dwarfs, neutron stars or black holes. The times of the explosions of intermediate (sun-like) stars can be determined by measuring the present brightness of the dwarfs. Not surprisingly the last two maxima of recordable near solar system star explosions took place during the presumably spiral arms driven glacial epochs in Eocene to present and Upper Jurassic times. Such near solar system star explosions may have been the source of intense neutrino showers, cosmic rays and star dust. This dust contained all kinds of chemical elements, including phosphorus and uranium. Such cosmic phosphorus may have supported, through fertilizing, the distribution of life on Earth additionally to local phosphorus resources via bloom of biota in lakes and oceans and the enhanced growth of plants on land across all climatic zones. Subsequently it maintained the development of petroleum source rocks of all organic matter types within black shales and coals. Via the distribution of remnants of exploding stars—mainly white dwarfs, but neutron stars and black holes have to be counted as well—a cosmic contribution can therefore casually linked to the deposition of petroleum source rocks on Earth, not only purely correlatively by their contemporaneous appearances. 展开更多
关键词 Cosmic Rays Cosmic Dust Milky Way spiral arms Stars PHOSPHORUS URANIUM Petroleum Source Rock
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超新星遗迹与银河系旋臂结构
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作者 宋国玄 《天文学报》 CSCD 北大核心 1999年第2期183-192,共10页
从分子云演化的过程来讨论银河系中可能存在的超新星遗迹数目.对银河系分子云的观测已经得到了许多可靠的数据.如果这一研究结果在分子云方面能使理论值和观测值相匹配,那么由此导得的超新星事件结果也有一定的可靠性.结果表明,在... 从分子云演化的过程来讨论银河系中可能存在的超新星遗迹数目.对银河系分子云的观测已经得到了许多可靠的数据.如果这一研究结果在分子云方面能使理论值和观测值相匹配,那么由此导得的超新星事件结果也有一定的可靠性.结果表明,在内银河系中,可能存在的超新星遗迹约为(775±12)τ5.旋臂结构并不会提高超新星的诞生率,它仅使超新星遗迹的分布有所变化,即在旋臂区域增加,而在臂间区域减少. 展开更多
关键词 银河系 旋臂 超新星遗迹 超新星
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