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浅析天文学科发展面临的挑战与应对
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作者 王彦博 《中文科技期刊数据库(全文版)自然科学》 2023年第7期115-118,共4页
天文学科的研究事关人类的发展,但在该领域我国之前一直处于较为落后的水平,一直未能建立起比较完善的研究体系,加之缺乏各种资源,使得我国天文学科的发展受到很大的限制,而这也影响了我国在相关技术领域的发展。如今,随着我国综合实力... 天文学科的研究事关人类的发展,但在该领域我国之前一直处于较为落后的水平,一直未能建立起比较完善的研究体系,加之缺乏各种资源,使得我国天文学科的发展受到很大的限制,而这也影响了我国在相关技术领域的发展。如今,随着我国综合实力与影响力的不断提升,我国天文学科发展迎来了难得的历史机遇,但同时也要清醒认识到所面临的挑战与困难,如此才能通过采取一系列的应对措施促进我国天文学科的快速发展。基于此,本文就从天文学科的概述出发,首先分析了国际天文学科的发展趋势及国内研究现状,接着重点探讨了新时代我国天文学科发展面临的机遇和挑战,并提出了一些可行性的应对措施,仅供参考。 展开更多
关键词 天文学科 研究现状 挑战 应对
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20O2年度天文学科科学基金面上项目评审工作回顾
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作者 董国轩 汲培文 《天文学进展》 CSCD 北大核心 2003年第1期87-90,共4页
介绍了2002年度天文学科科学基金申请、资助的基本情况,并对某些结果进行了分析。
关键词 2002年 天文学科 申请 资助 科学研究工作 自然科学基金
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一门新兴的交叉天文学科 ——“天地生”
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作者 郭德才 《科学之友》 2001年第12期16-18,共3页
近代科学的发展已经有近百年的历史了,但最初每一门学科的研究几乎都是封闭单一的.随着科学的发展和深入,人们逐渐发现很多学科并不是孤立的,它们之间都存在一定影响和物质能量交换的关系.浩瀚的宇宙用斑斓绚丽的星烁展示着它的恢宏气势... 近代科学的发展已经有近百年的历史了,但最初每一门学科的研究几乎都是封闭单一的.随着科学的发展和深入,人们逐渐发现很多学科并不是孤立的,它们之间都存在一定影响和物质能量交换的关系.浩瀚的宇宙用斑斓绚丽的星烁展示着它的恢宏气势,它那无穷的能量和运动也同时在影响着地球和人类的健康.所谓"天地生"这门学科,既是在现代科学发展基础上将天文、地球、生物作为一个相互联系、相互作用的整体进行多学科的综合研究,它包含有天文地质学、天文地震学、天文气象学、天文医学、历史自然学、灾害学、生物学等许多新兴的学科. 展开更多
关键词 太阳活动 地球灾害 人体健康 交叉天文学科 天体活动 影响研究
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新时代我国天文学科发展的思考 被引量:3
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作者 刘强 颜景志 董国轩 《中国科学基金》 CSCD 北大核心 2019年第5期520-524,共5页
本文从天文学的特点、国际天文学发展态势和国内研究现状出发,分析了目前我国天文学研究面临的机遇和挑战。针对这些机遇和挑战,建议自然科学基金应该支持建造一批有竞争力的观测设备、支持天文交叉学科发展并增加天文学科资助的渠道,... 本文从天文学的特点、国际天文学发展态势和国内研究现状出发,分析了目前我国天文学研究面临的机遇和挑战。针对这些机遇和挑战,建议自然科学基金应该支持建造一批有竞争力的观测设备、支持天文交叉学科发展并增加天文学科资助的渠道,加强学科布局,扩大人才队伍的培养,促进我国天文学科的快速发展。 展开更多
关键词 国家自然科学基金 天文学科 机遇 挑战
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赫歇尔空间天文台科学地面段软件开发管理方法的研究 被引量:1
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作者 张洁 黄茂海 《天文研究与技术》 CSCD 2015年第2期212-218,共7页
国内空间项目软件管理方法已经不能满足当前日益复杂的地面应用系统的要求。深入研究了具有国际领先水平的赫歇尔(Herschel)空间天文台科学地面段的软件开发管理方法。赫歇尔科学地面段基于迭代模型的分支开发的特点,切实可行的软件管... 国内空间项目软件管理方法已经不能满足当前日益复杂的地面应用系统的要求。深入研究了具有国际领先水平的赫歇尔(Herschel)空间天文台科学地面段的软件开发管理方法。赫歇尔科学地面段基于迭代模型的分支开发的特点,切实可行的软件管理计划以及基于用例需求的开放管理方式改变了地面段总是处于整个工程建设的末端的现状,而是从载荷研制阶段就开始工作,而且面对频繁的需求变更,始终保持高效的工作状态,这些在国内空间项目中是前所未有的。本研究给国内空间项目的软件开发提供了新的思路和方法。 展开更多
关键词 空间天文学其他学科 软件开发管理 过程模型 迭代开发 需求管理 用例
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卫星定位精度对在轨甚低频干涉测量影响分析 被引量:2
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作者 张墨 黄茂海 颜毅华 《天文研究与技术》 CSCD 2014年第4期362-368,共7页
由于地球电离层的阻挡以及其他干扰,在地面难以进行有效的甚低频天文观测,而使用搭载于绕地或绕月轨道卫星上的甚低频天线进行干涉观测会大大提高观测灵敏度和角分辨率。卫星定位精度会影响观测数据的处理结果,进而影响成图质量,并且会... 由于地球电离层的阻挡以及其他干扰,在地面难以进行有效的甚低频天文观测,而使用搭载于绕地或绕月轨道卫星上的甚低频天线进行干涉观测会大大提高观测灵敏度和角分辨率。卫星定位精度会影响观测数据的处理结果,进而影响成图质量,并且会大幅影响飞行项目的复杂度和总成本。首先分析卫星姿态控制精度和星间基线测量精度对绕地轨道甚低频干涉观测的影响,之后对干涉观测中信号延时误差进行仿真,研究延时误差与数据相关处理中条纹搜索范围之间的关系,并对数据计算速度需求进行估算。分析和仿真结果可以辅助相关空间甚低频观测项目总体方案的制定和工程指标的优化。 展开更多
关键词 空间天文学其他学科 甚低频 仿真 卫星定位 条纹搜索
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Ottoman Mathematicians and Astronomers
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作者 Malahat Abdullayeva 《Sino-US English Teaching》 2018年第1期49-55,共7页
The article deals with the scientists in the Ottoman Empire. The readers will get interesting information about the life and practices of those who dedicated their whole life to the development of science, such as Ott... The article deals with the scientists in the Ottoman Empire. The readers will get interesting information about the life and practices of those who dedicated their whole life to the development of science, such as Ottoman mathematicians and astronomer Rumi Kadizade from Bursa, Ali Kushchu, Mirim Chalabi, Takiyuddin Bin Maruf-i, Gelenbevi Ismail Efendi, Hoca Ishak Efendi, and Huseyin Tevfik Pasha. 展开更多
关键词 Ottoman Empire MATHEMATICS ASTRONOMY OBSERVATORY
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The Italic School in Astronomy: From Pythagoras to Archimedes 被引量:1
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作者 Giuseppe Boscarino 《Journal of Physical Science and Application》 2014年第6期385-392,共8页
It is argued that it has not yet been able to value the historical, philosophical and epistemological travail, represented by the filth and fourth centuries BC of the ancient Greek world, which preceded the highest sc... It is argued that it has not yet been able to value the historical, philosophical and epistemological travail, represented by the filth and fourth centuries BC of the ancient Greek world, which preceded the highest scientific heritage, represented by the so-called golden age of Euclid, Archimedes and Apollonius, Ⅲ-Ⅱ century BC. Well, it is believed that with our complex concept of tradition of thought within which we insert not only epistemological concepts but also philosophical principles, historical and social frameworks, in stasis or in strong movement, processed by us, it is possible better interpret that happy moment of scientific constructions of the third and second century BC, as a result of the valorization of the deep travail and serious battle that preceded it between the fourth and fifth century BC. It is investigated in particular in our paper the development of astronomical thought between the fifth and fourth centuries BC, in the ancient Greek thought, and at last a particular presumed criticism by Archimedes in his Sandreckoner to Aristarchus. 展开更多
关键词 Scientific theories Traditions of thought.
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Philosophical Study of Scientific Proof
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作者 Bondarenko Stanislav Borisovich 《Journal of Philosophy Study》 2015年第1期24-28,共5页
The scientific proof is the highest type of the rational proof. The mankind is looking for the best technology of the reasonable demonstration. What is a proof?. What is a scientific proof?. Philosophical investigat... The scientific proof is the highest type of the rational proof. The mankind is looking for the best technology of the reasonable demonstration. What is a proof?. What is a scientific proof?. Philosophical investigations of proofs have the long history. Philosophy is exploring physics, mathematics, astronomy, biology, history, and so on. Science demands strict proofs. Science uses the specific methods as the optimum technologies for the achievement of the truth. Strictness of the proof depends on the aim algorithm: the distribution of the functions between parts of the proof. The beginning stage, the middle parts, and the ending stage are the unit of the proof. Philosophy can make the correct model of the scientific proof only! Science and its methodology develop and the growth of knowledge has not the finish. The rational ideals improve continually. Science is looking for the criterion of the demonstrative strictness. The adaptation algorithm of the scientific method is the best technology for the achievement of the truth. 展开更多
关键词 SCIENCE PROOF model method UNIT ALGORITHM
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Estimation of the inter-frequency clock bias for the satellites of PRN25 and PRN01 被引量:10
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作者 LI HaoJun ZHOU XuHua +1 位作者 WU Bin WANG JieXian 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS 2012年第11期2186-2193,共8页
We present two efficient approaches,namely the epoch-differenced(ED) and satellite-and epoch-differenced(SDED) approaches,for the estimation of IFCBs of the two Block IIF satellites.For the analysis,data from 18 stati... We present two efficient approaches,namely the epoch-differenced(ED) and satellite-and epoch-differenced(SDED) approaches,for the estimation of IFCBs of the two Block IIF satellites.For the analysis,data from 18 stations from the IGS network spanning 96 d is processed.Results show that the IFCBs of PRN25 and PRN01 exhibit periodical signal of one orbit revolution with a magnitude up to 18 cm.The periodical variation of the IFCBs is modeled by a sinusoidal function of the included angle between the sun,earth and the satellite.The presented model enables a consistent use of L1/L2 clock products in L1/L5-based positioning.The algorithm is incorporated into the MGPSS software at SHAO(Shanghai Astronomical Observatory,Chinese Academy of Sciences) and is used to monitor the IFCB variation in near real-time. 展开更多
关键词 triple-frequency signals precise point positioning inter-frequency clock bias
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WORLD
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《Beijing Review》 2016年第7期8-9,共2页
THE UNITED STATES U.S.scientists announce on February 11 that they have detected the existence of gravitational waves through the Laser Interferometer GravitationalWave Observatory in Livingston,Louisiana(pictured ab... THE UNITED STATES U.S.scientists announce on February 11 that they have detected the existence of gravitational waves through the Laser Interferometer GravitationalWave Observatory in Livingston,Louisiana(pictured above). 展开更多
关键词 announce gravitational Einstein WORLD agreed alliance launch visitors military triggered
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Activity of comet 103P/Hartley 2 from September 30 to November 04, 2010
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作者 SHI JlanChun ZHAO HaiBin MA YueHua 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS 2012年第8期1515-1518,共4页
The CCD photometric observation of comet 103P/Hartley 2 with broadband optical filters was carried out at Xuyi Station of Purple Mountain Observatory, Chinese Academy of Sciences by use of Near Earth Object Telescope ... The CCD photometric observation of comet 103P/Hartley 2 with broadband optical filters was carried out at Xuyi Station of Purple Mountain Observatory, Chinese Academy of Sciences by use of Near Earth Object Telescope (NEOT). We monitored the comet from September 30 to November 4, 2010 and investigated the variation of activities. The Afp parameter derived from our r broadband data varies from 46.0 to 126.0 cm and increases with time. The dust production rate in terms of Afp was measured and a tentative calculation of the dust (or gas) loss-rate of nucleus was executed under the assumption that the nucleus of comet 103P/l-lartley 2 is spherical. The r-band image and the surface brightness profile taken on September 30, 2010 was measured and the gradient of surface brightness profile of 103P/Hartley 2 showed m 〈 -1.5, 展开更多
关键词 comets 103P/Hartley 2 ACTIVITY
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