天文望远镜

tiān wén wànɡ yuǎn jìnɡ
  • astronomical telescope
天文望远镜天文望远镜
天文望远镜 [tiān wén wàng yuǎn jìng]
  • [astronomical telescope] 为观测天体设计的望远镜,不需要倒像转正系统

  1. 基于Matlab的天文望远镜实时位置仿真显示

    Simulate Display of Real-time Position of Astronomical Telescope based on Matlab

  2. X射线天文望远镜的进展

    The development of X-ray astronomical telescopes

  3. 权势集团1983年意识到X星入境,由他们自己的红外天文望远镜通过被发送到云层之上的红外气球看到。

    The establishment was aware that Planet X was inbound by1983 , confirmed by their own IRAS sightings via an infrared balloon sent above the clouds .

  4. 在过去十年间,钱德拉X射线天文台经常协同其他天文望远镜对“蟹状星云”进行联合观测。

    In the past decade , the Chandra X-ray Observatory , often in conjunction with other astronomical telescopes on the " Crab Nebula " in joint observation .

  5. 硬X射线调制望远镜(HXMT)是我国正在研制的用于空间硬X射线观测的天文望远镜。

    Hard X-ray Modulation Telescope ( HXMT ) is an astrophysics telescope that is being studied in China .

  6. 基于Stewart平台的馈源位姿主动减振定位机构的控制是五百米口径球面射电天文望远镜(FAST)项目实现的关键。

    Active vibration control of the feed support system based on Stewart platform is essential for constructing a five-hundred-meter aperture spherical telescope ( FAST ) successfully .

  7. 简述大型天文望远镜对传感器的需求,重点介绍了CCD传感器、波面传感器和光栅传感器等在大型天文望远镜中应用。

    Requirements of telescope and main technological features of sensor are introduced . CCD camera , wavefront sensor and grating sensor etc application for large astronomical telescope are described .

  8. X射线衍射光学元器件在激光惯性约束聚变,天文望远镜,同步辐射,EUV光刻等领域有着广泛应用。

    X-ray diffraction optical elements have a broad application in the field of the inertial confinement fusion , astronomical telescopes , synchrotron radiation and EUV lithography .

  9. 关于φ2.2m天文望远镜坯的流体力学计算

    On the fluid dynamics calculation of the φ 2.2m astronomical telescope lens

  10. 2.4m天文望远镜光学系统的设计及副镜检验的几种可能方案

    Optic System Design of a 2.4m Class Telescope and Several Methods for Testing the Secondary Mirror

  11. 本文介绍了球载硬X射线空间高能天文望远镜HAPI-4系统探测器平台即吊舱系统的状态空间模型。

    This paper introduces the state-space model of the detecting platform of the balloon-borne hard X-ray astronomical telescope HAPI-4 system . and its LQR designing method .

  12. 2.16m天文望远镜观测室工程的施工技术

    Construction Techniques of the 2 . 16m Astronomical Telescope Observation Station Engineering

  13. 作者研究了φ2.2m天文望远镜坯的流体动力学问题。

    Fluid dynamics for the φ 2.2m astronomical telescope lens has been studied by the anthors .

  14. 近年来,随着多层膜技术的深入发展,多层膜反射镜已在软X射线天文望远镜,软X射线显微术,X射线投影光刻,同步辐射,等离子体诊断等许多领域内成功的获得了应用。

    In recent years , with the development of multilayer technology , the multilayer mirror has successfully been used in the fields of X-ray astronomy telescope , X-ray microscopy , X-ray project lithography , synchrotron , plasma diagnosis and so on .

  15. 并且,在国家科技部,云南省政府,以及中科院的支持下,2m级天文望远镜项目在2000年12月获得立项。

    Supported by the Ministry of Science and Technology , the Government of Yunnan Province and the Chinese Academy of Sciences , a 2m class telescope project was granted .

  16. Stockes参数偏振光测量在空间天文望远镜中的应用

    Principle of Stockes Parameters Polarized Light Measurement with It 's Usage in SST

  17. 而国内普遍使用基于PC的Windows操作系统,并将其应用于天文望远镜的控制和数据采集(例如云南天文台1米望远镜、上海天文台佘山天文观察站1.56米望远镜的控制和采集系统)。

    However , windows operating system based on personal computer are wildly used in our country and applied to the control and data collection for astronomical telescope , example for 1m telescope at Yunnan Observatory and 1.56m telescope at Shanghai Astronomical Observatory ( SHAO ) .

  18. 通光口径2.16m天文望远镜凹双曲面主镜的磨制工艺

    The technology of the concave hyperbolic primary mirror of the effective aperture 2.16 m astronomical telescope

  19. 结合实际测试结果,介绍了大天区面积多目标光纤光谱天文望远镜(LAMOST)低色散光谱仪所使用的科学级CCD相机的系统设计与检测技术。

    A scientific CCD camera for the low-dispersion spectrograph of large sky area multi-object fiber spectroscopic telescope ( LAMOST ) was introduced along with the test and analysis of its performance .

  20. 文中以通光口径2.16m天文望远镜为例,给出了光路调整图。

    Finally , as an example , the alignment diagram of the clear aperture 2.16m astronomical telescope is given .

  21. EPICS是用于开发分布式实时控制系统的软件工具包,广泛应用于粒子加速器、高能物理实验、天文望远镜等大型科学实验设备的控制系统的开发。

    EPICS is a set of software tools and applications used worldwide to develop distributed real-time control systems for scientific facilities such as particle accelerators , telescopes and other large scientific experiments .

  22. 英国RDF电视传媒和社交网站Bebo使用乌克兰的无线电天文望远镜将以无线电方式收集的500条来自大众的信息发送了给了Gliese581。

    Documentary-maker RDF and social-networking site Bebo used a radio telescope in Ukraine to send a powerful focused beam of information - 500 messages from the public in the form of radio waves - to Gliese 581 .

  23. 大天区面积多目标光纤光谱天文望远镜(LAMOST)是一架我国科学家自主创新设计和研制的反射施密特望远镜,是世界上光谱获取率最高的望远镜。

    The Large Sky Area Multi-Object Fiber Spectroscopic Telescope ( LAMOST ) is an innovative reflecting Schmidt telescope , promising a very high spectrum acquiring rate of several ten-thousands of spectra per night .

  24. 然而,Tylenda却在偶然的机会中发现,原来在波兰首都华沙的天文台里的一个天文望远镜一直观测着这一区域。

    However Mr Tylenda then realised that an observatory in the Polish capital Warsaw had , by chance , been pointing its lens at the region for several years .

  25. 该文的研究成果对于正在研制中的我国大科学工程项目大天区面积多目标光纤光谱天文望远镜LAMOST的环境监控系统的设计具有相当的参考价值。

    The research practice has particularly provided valuable experience for the design of environmental monitor system of the ongoing large sky area multi-object fiber spectroscopic Telescope ( LAMOST ), which is one of the large scientific projects in China .

  26. 虽然它是温度最冷的地外行星中被天文望远镜直接捕捉到影像的一个(而不是在从其宿星前经过时被检测到一抹暗淡的星光),HD131399Ab星球上的平均温度超过华氏1000度,远超人类耐热标准。

    And while it 's one of the coldest exoplanets ever to be directly imaged by a telescope ( rather than detected as a result of the dimming of starlight as it passes in front of its host star ) , HD 131399Ab is very hot by human standards . The average temperature exceeds 1000 degrees Fahrenheit .

  27. 光学天文望远镜用微位移驱动器机构研究综述

    Review of Mechanical Structure of Micro-displacement Actuator for Optical Astronomical Telescope

  28. 装载着可以观察红外辐射的天文望远镜的人造卫星。

    A satellite equipped with a telescope to observe infra-red radiation .

  29. 波前检测是天文望远镜自适应光学中的重要环节。

    Wavefront sensing is a crucial part of adaptive optics technology .

  30. 系统仿真在天文望远镜设计中的应用综述

    Application Review of System Simulation Technique in Astronomical Telescope Design