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Acceleration of galactic cosmic rays 银河宇宙射线的加速
Pub Date : 2019-12-02 DOI: 10.1393/ncr/i2019-10166-0
P. Blasi
More than a century ago it was discovered that the Earth is bombarded by a penetrating radiation of cosmic origin, whose flux was later found to be dominated by charged particles. The discovery of cosmic rays led to many questions about their origin and about the way that they reach us from large distances. Here I will summarize some recent developments in our understanding of the acceleration mechanisms that energize a small number of thermal particles to highly non-thermal energies, with special attention on diffusive acceleration at supernova remnant shocks.
一个多世纪以前,人们发现地球受到来自宇宙的穿透辐射的轰击,后来发现其通量主要是带电粒子。宇宙射线的发现引发了许多关于它们的起源以及它们从很远的地方到达我们的方式的问题。在这里,我将总结我们对加速机制的一些最新进展,这些加速机制将少量热粒子激发为高度非热能量,特别关注超新星残余激波的扩散加速。
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引用次数: 0
Entropy in self-assembly 自组装中的熵
Pub Date : 2019-11-05 DOI: 10.1393/ncr/i2019-10165-1
Francesco Sciortino
Colloidal systems show beautiful examples of how entropy can lead to self-assembly of ordered structures, challenging our perception of disorder. In fact, dispersion of hard colloidal particles, systems in which by default entropy is the only thermodynamic driving force, displays both translational and orientational order on increasing density. Entropy is also a fundamental concept for describing effective interactions between colloidal particles. In several cases, entropy maximization generates strong attractive forces, capable of inducing condensation and sometimes crystallization. These entropic forces can even be exploited to drive colloids in specific locations or to orient them in the build-up of supracolloidal aggregates. Depletion interactions and combinatorial contributions are two important manifestations of these forces. Entropy also plays a leading role in systems exploring the bottom of their potential energy surface. In patchy colloids, particles interacting with highly anisotropic and localized potentials, ground-state structures are often degenerate in energy, leaving entropy to decide the thermodynamically stable polymorph. A striking result is the possibility of generating colloidal “liquids” thermodynamically more stable than colloidal “crystals” even at vanishing temperature.
胶体系统展示了熵如何导致有序结构的自组装,挑战我们对无序的认知。事实上,在默认熵是唯一热力学驱动力的系统中,硬胶体颗粒的分散随密度的增加同时显示平动和定向顺序。熵也是描述胶体粒子之间有效相互作用的基本概念。在一些情况下,熵的最大化会产生强大的吸引力,能够引起凝结,有时还会引起结晶。这些熵力甚至可以用来驱动特定位置的胶体,或者在超胶体聚集体的形成中使它们定向。耗竭相互作用和组合贡献是这些力的两个重要表现。熵在系统探索其势能面底部的过程中也起着主导作用。在斑块状胶体中,粒子与高度各向异性和局域电位相互作用,基态结构往往在能量上简并,留下熵来决定热力学稳定的多晶型。一个惊人的结果是,即使在消失的温度下,也有可能产生比胶体“晶体”更稳定的胶体“液体”。
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引用次数: 0
Astrometry in the 21st century. From Hipparchus to Einstein 21世纪的天体测量学。从喜帕恰斯到爱因斯坦
Pub Date : 2019-10-14 DOI: 10.1393/ncr/i2019-10164-2
Mariateresa Crosta
Astrometry is that fundamental part of astronomy which allows to determine the geometric, kinematical, and dynamical properties of celestial objects, including our own Galaxy, which is assembled and shaped by gravity. The knowledge of star positions was already important at the times of Hipparchus (190–120 BC) and his predecessors, Timocharis and Aristillos. Their cataloging (approximately 150 years earlier) of star positions enabled Hipparchus to update the observations with a precision of nearly half a degree and thus to discover the phenomenon of equinox precession. Nowadays a big jump is mandatory: positions, motions, and distances exist in the realm of the Einstein Theory and null geodesics represent our unique physical links to the stars through a curved space-time, namely a varying background geometry. Astrometry must be equipped with all of the proper tools of General Relativity to define the observables and the measurements needed for compiling astronomical catalogs at the microarcosecond accuracy and beyond. The astrometry of the 21st century, endowed with a fully relativistic framework, is fully fledged for new potential applications in astrophysics, can lead the way to forefront discoveries in fundamental physics, and is becoming the pillar of Local Cosmology. In this respect, it is more appropriate, in the 21st century, to refer to it as “Gravitational Astrometry”.
天体测量学是天文学的基础部分,它可以确定天体的几何、运动学和动力学特性,包括我们自己的星系,它是由引力聚集和塑造的。在喜巴恰斯(公元前190-120年)和他的前任提莫查里斯和阿里斯蒂略时代,关于恒星位置的知识已经很重要了。他们对恒星位置的编目(大约早了150年)使喜帕恰斯能够以接近半度的精度更新观测结果,从而发现了春分岁差现象。如今,一个大的跳跃是必须的:位置、运动和距离存在于爱因斯坦理论的领域,零测地线代表了我们通过弯曲的时空与恒星的独特物理联系,即变化的背景几何。天体测量学必须配备广义相对论的所有适当工具,以定义可观测到的天体,并进行精确到微秒以上的天文编目所需的测量。21世纪的天体测量学被赋予了一个完全相对论的框架,在天体物理学中有了新的潜在应用,可以引领基础物理学的前沿发现,并正在成为局部宇宙学的支柱。在这方面,在21世纪,将其称为“引力天体测量学”更为合适。
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引用次数: 0
Inversion of earthquake rupture process: Theory and applications 地震破裂过程反演:理论与应用
Pub Date : 2019-09-02 DOI: 10.1393/ncr/i2019-10162-4
Yun-tai Chen, Yong Zhang, Li-sheng Xu
We present the theory and methods of earthquake rupture process inversion by using seismic and geodetic data, and their applications to scientific researches and earthquake emergency responses. It is shown that the knowledge obtained from these studies has much improved our understanding of the complexities of the earthquake source and causative mechanism of the earthquake disaster, and is of important reference value in earthquake disaster mitigation such as rapid earthquake emergency response. Especially since the 2008 Mw7.9 (MS8.0) Wenchuan, Sichuan, earthquake, fast and routine determination of the earthquake rupture process has been performed for significant earthquakes (MS ≥ 6.5 in China and MS ≥ 7.5 worldwide), and the results obtained are timely reported to the authorities and released to the public on the web site. The time consumed by the inversion has been reduced from more than 5 hours in 2009 to approximately 1–3 hours at present. The timely released rupture model was routinely used by the China Earthquake Administration and other authorities during the earthquake emergency responses period for destructive earthquakes, such as the 2010 Mw6.9 Yushu earthquake, the 2013 Mw6.6 Lushan earthquake, the 2014 Mw6.1 Ludian earthquake, and the 2015 Mw7.8 Gorkha, Nepal, earthquake, among the others.
介绍了利用地震和大地测量资料反演地震破裂过程的理论和方法,及其在科学研究和地震应急响应中的应用。研究结果表明,这些研究成果大大提高了我们对震源复杂性和地震灾害成因机制的认识,对地震快速应急响应等地震减灾具有重要的参考价值。特别是自2008年四川汶川Mw7.9 (MS8.0)地震以来,对重大地震(中国≥6.5,世界≥7.5)进行了地震破裂过程的快速常规测定,并及时向有关部门报告结果,并在网站上向公众发布。反演时间由2009年的5个多小时减少到目前的1-3小时左右。及时发布的断裂模型被中国地震局和其他有关部门在地震应急响应期间经常用于破坏性地震,如2010年玉树6.9级地震、2013年芦山6.6级地震、2014年鲁甸6.1级地震和2015年尼泊尔廓尔喀7.8级地震等。
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引用次数: 0
The Metre Convention of 1875: A Commentary and new English edition 1875年《米制公约》评注及新英文版
Pub Date : 2019-07-01 DOI: 10.1393/ncr/i2019-10160-6
Terry Quinn
In my Commentary on the Metre Convention of 1875, modified by the second Convention in 1921, I examine its mission “to assure the international unification and perfection of the metric system” set out in the Preamble to the 1875 Convention and show how this continues to be its principal aim, with the metric system now being the International System of Units, SI. I examine the modern roles of the three organs of the Convention, the General Conference on Weights and Measures, the International Committee for Weights and Measures and the International Bureau of Weights and Measures—the permanent international scientific institute at Sevres. I discuss the interpretation of many of the key Articles of the Conventions, drawing upon decisions made by General Conferences. I discuss the recent interpretation of one of these by the International Committee. I draw attention to the 1960 draft of a proposed new Convention, much discussed at the 11th General Conference in 1960 but never adopted, which would have considerably eased recent financial difficulties by removing the requirement for unanimity in financial decisions. The new English edition of the Convention, in the Appendix, is the first complete and up to date English text to include both the Preamble to the 1875 Convention and the text of the second Convention of 1921.
在我的《1875年米制公约评注》中,我考察了1875年公约序言中提出的“确保公制在国际上的统一和完善”的使命,并说明了公制现在是国际单位制SI,这仍然是它的主要目标。我考察了公约的三个机构——国际度量衡大会、国际度量衡委员会和国际度量衡局——位于塞夫尔的常设国际科学机构——的现代作用。我根据大会作出的决定,讨论对《公约》许多关键条款的解释。我要讨论国际委员会最近对其中一项的解释。我提请注意1960年提出的一项新公约草案,该草案在1960年第十一届大会上进行了大量讨论,但从未获得通过,该草案取消了在财务决定中必须一致通过的要求,将大大缓解最近的财政困难。附录中的《公约》新英文版是第一个完整的最新英文文本,既包括1875年《公约》的序言,也包括1921年《第二公约》的案文。
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引用次数: 0
A unique mission: Cassini-Huygens, the Orbiter, the descent Probe and the cruise science 一个独特的任务:卡西尼-惠更斯号,轨道飞行器,下降探测器和巡航科学
Pub Date : 2019-06-27 DOI: 10.1393/ncr/i2019-10159-y
E. Flamini, A. Adriani, J. W. Armstrong, F. Capaccioni, G. Filacchione, L. Iess, G. Mitri, S. Viviano
The Cassini-Huygens mission has characterized the Solar System exploration scenario for more than 30 years, from when it was conceived until the completion of its long life. Its legacy is an enormous amount of high quality scientific data and astonishing images of the Saturn system and its moons, Titan first. Also, the mission has been the gymnasium where new technologies and procedures have been discussed, developed and after adopted by many other missions. Cassini-Huygens also played a great role in allowing a new generation of scientists and engineers to increase their knowledge and skills, merging the already matured experience of a generation, formed on previous missions as Voyager, with a new generation belonging to many different countries. The international scenario that allowed the realization of the mission is the other distinguishing character of this adventure, led by the partnership of three space agencies, NASA with the Jet Propulsion Laboratory first, the European Space Agency-ESA for Huygens and the Italian Space Agency-ASI. This cooperative environment allowed both ESA and ASI to enter at best in the environment of the deep-space planetary missions and also provided the opportunity for other 15 nations to have their scientist on board and contributing to the mission. A cooperative effort, well guided and harmonized by the Project Science Group, lasted till the very end of the mission when the Cassini Grand Finale was played with the last plunge into the Saturn atmosphere. Hereafter, the mission is described including some details on the technical aspects of the Cassini spacecraft, the Huygens probe, the science instruments part of their payload and the science results are summarized with a special emphasis on the Italian contribution. This paper focuses on the science results in the cruise phase, where radio science experiments testing different aspects of relativistic gravity were performed. In particular, we describe the use of the novel Cassini radio system (based on Ka band frequencies, 32–34 GHz) to test the space components of the metric in the Solar System and a search of low-frequency gravitational waves, with a set of extensive observations in 2001 and 2002. The Cassini radio signal was tracked just prior to the final plunge into Saturn’s atmosphere (15 September 2017) from a new configuration of the Sardinia Radio Telescope called “Sardinia Deep Space Antenna”. The Venus and Jupiter fly-bys offered the opportunity to calibrate the VIMS instrument and to carry out new science observations.
卡西尼-惠更斯号任务从构思到完成漫长的生命周期,已经有30多年的太阳系探索历程了。它留下了大量高质量的科学数据和土星系统及其卫星的惊人图像,首先是土卫六。此外,特派团一直是讨论、开发新技术和程序的体育馆,并被许多其他特派团采用。卡西尼-惠更斯号还发挥了重要作用,使新一代科学家和工程师能够增加他们的知识和技能,将在旅行者号之前的任务中形成的已经成熟的经验与来自许多不同国家的新一代科学家和工程师融合在一起。这次冒险的另一个显著特点是,这次冒险是由三个空间机构合作领导的,美国国家航空航天局(NASA)首先是喷气推进实验室,欧洲航天局(esa)负责惠更斯号,意大利航天局(asi)负责。这种合作环境使欧空局和ASI充其量只能进入深空行星任务的环境,也为其他15个国家提供了让他们的科学家参与并为任务作出贡献的机会。在项目科学小组的指导和协调下,一项合作努力一直持续到任务的最后一刻,卡西尼号最后一次进入土星大气层时,奏响了压轴曲。接下来,对这次任务进行了描述,包括卡西尼号航天器、惠更斯号探测器、科学仪器部分有效载荷的技术方面的一些细节,以及对科学结果的总结,特别强调了意大利的贡献。本文重点介绍了巡航阶段的科学成果,在巡航阶段进行了无线电科学实验,测试了相对论引力的不同方面。特别是,我们描述了使用新的卡西尼无线电系统(基于Ka波段频率,32-34 GHz)来测试太阳系中度量的空间分量和搜索低频引力波,并在2001年和2002年进行了一系列广泛的观测。卡西尼号的无线电信号是在最后一次进入土星大气层之前(2017年9月15日),由撒丁岛射电望远镜的新配置“撒丁岛深空天线”跟踪的。金星和木星的飞掠为校准VIMS仪器和进行新的科学观测提供了机会。
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