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Yang Kejun 《时间频率学报》1995,(1)
本文分析了利用中国科学院陕西天文台的流星雷达进行人为空间碎片监测的可能性.详细计算了到达接收机的回波的信噪比S/N依赖于目标散射横截面。和高度距离R的关系。理论计算表明,利用陕西天文台的流星雷达完全有可能监测在200km至1200km的高度范围内,半径大于0.5m的人为空间碎片. 相似文献
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用陕西天文台流星雷达监测人为空间碎片可能性的分析 总被引:1,自引:0,他引:1
本文分析了利用中国科学院陕西天文台的流星雷达进行人为间空碎片监测的可能性。详细计算了到达接收机的回波的信噪比S/N依赖于目标散射截面σ和高度距离R的关系。理论计算表明,利用陕西天文台的流星雷达完全有可能监测在200km至1200km的高度范围内,半径大于0。5m的人为空间碎片。 相似文献
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阐述了虚拟天文台的科学目标和一些基于虚拟天文台的成功范例及其优越性,以此显示创建虚拟天文台和构想新的研究范例的必要性,同时也说明虚拟天文台是由需求带动发展,并逐步由虚拟变为现实的研究途径。作为21世纪新的研究平台,虚拟天文台将在知识和技术等方面对天文学家提出新的挑战,提供新的机遇。 相似文献
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阐述了虚拟天文台的科学目标、可能的基于虚拟天文台的项目、虚拟天文台的作用和意义;着重介绍了目前虚拟天文台项目开发的各种工具及应用.随着各种工具的开发、集成和应用,虚拟天文台的功能将越来越完善,其成功的科学范例再次显示了虚拟天文台的优越性,标志着虚拟天文台正在从“概念”转向“操作”,由“技术”向“科学”靠近,以“科学”为主旋律前进。虚拟天文台将成为天文学家科研工作必不可少的一部分。 相似文献
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中国虚拟天文台研发策略与重点 总被引:5,自引:3,他引:2
由于不同的天文和技术背景,不同的虚拟天文台项目采取了不同的研究策略。本文首先介绍了国际上几个典型虚拟天文台项目的研发目标和工作重点;然后讨论了包括中国虚拟天文台在内的小型虚拟天文台项目在研发方面的优势和劣势。中国虚拟天文台项目根据自身所处的具体情况确定自己将走应用路线,争取在某些领域取得突破,研发重点包括五个方面:China-VO系统平台建设、国内外天文数据的统一访问、现有天文工具的虚拟天文台集成、天文设备的虚拟天文台集成、虚拟天文台基础上的公众教育。 相似文献
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光污染和光学天文台址保护 总被引:1,自引:0,他引:1
讨论了天光背景对光学天文台的背景,综述了造成光污染的主要途径,介绍了防止光污染的几个主要国际组织和国际上对天文台址的保护立法,提出了减少污染的主要措施。为国内进行光学天文台址保护采取措施以至(国家的或者地方的)立法提供参考。 相似文献
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The upwelling radiation at the top of the atmosphere is computed over a circular lake which is located in the uniform Lambert surface, using a modified version of the doubling-adding method. The radiance over the lake is discussed with respect to the atmospheric effect. The radius of the lake is assumed to be 0.5, 1, and 3 km. The observational site is located at altitude 30 km. The zenith of the observational site is located in the plane which is determined by the zenith of the center of the lake and incident solar direction. The zenith angle of the observational site to the center of the lake is fixed to 6.28°. The atmosphere is assumed to be homogeneous, which is composed of aerosol and molecule, where the model aerosol is of the oceanic or the water soluble types.Numerical simulation exhibits an extraordinary effect near the lake. The radiance of the lake against the surrounding depends upon the albedo of the surrounding surface. It increases with the increase of the size of the lake and decreases with the optical thickness. At large optical depth, the radiance depends upon the aerosol characteristics. It shows little dependence on the solar zenith angle if less than 60°. 相似文献
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Shantikumar S. Ningombam S. Kathiravan P. S. Parihar E. J. L. Larson Sharika Mohanan Dorje Angchuk Sonam Jorphel K. E. Rangarajan K. Prabhu 《Experimental Astronomy》2017,43(2):145-165
The present work discusses astronomical site survey reports on dust content, vertical distribution of atmospheric turbulence, precipitable water vapor (PWV), surface and upper-air data, and their effects on seeing over the Indian Astronomical Observatory (IAO) Hanle. Using Laser Particulate Counter, ambient dust measurements at various sizes (0.3 μm to 25 μm) were performed at various locations at the site during November 2015. Estimated volume concentration for the particle size at 0.5 μm was around 10,000 per cubic foot, which is equivalent to ten thousand class of clean room standard protocol. During the measurement, surface wind speed varied from 0-20 m s ?1, while estimated aerosol optical depth (AOD) using Sky radiometer (Prede) varied from 0.02-0.04 at 500 nm, which indicates the site is fairly clean. The two independent measurements of dust content and aerosol concentrations at the site agreed well. The turbulence or wind gust at the site was studied with wind profiles at three different heights above the ground. The strength of the wind gust varies with time and altitude. Nocturnal temperature across seasons varied with a moderate at summer (6?8 °C) and lower in winter (4?5 °C). However, the contrast between the two is significantly small due to cold and extremely dry typical climatic conditions of the site. The present study also examined the effects of surface and upper-air data along with Planetary Boundary Layer (PBL) dynamics with seeing measurement over the site. Further, a comparative study of such observed parameters was conducted with other high altitude astronomical observatories across the globe. 相似文献
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M. Jurado Vargas P. Merchán Benítez F. Sánchez Bajo A. Astillero Vivas 《Astrophysics and Space Science》2002,279(3):261-269
In order to determine the atmospheric extinction at Physics Department Astronomical Observatory of the University of Extremadura, located at Badajoz (Spain), several stars were observed during some clear nights of atmospheric stability in the period 1998–2000, at optical wavelengths corresponding to the filters of the Kron-Cousins and Strömgren photometric systems. The determination of the extinction coefficients was made by assuming the Bouguer's law, which was shown to be a good approximation for this study. The results exhibited temporal variations and can be considered to be associated with clean atmospheres at locations of low altitude. 相似文献
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V. Kornilov S. Ilyasov O. Vozyakova Yu. Tillaev B. Safonov M. Ibragimov N. Shatsky Sh. Egamberdiev 《Astronomy Letters》2009,35(8):547-554
We present the results of our 2005–2007 campaign to measure the vertical distribution of optical turbulence above Mount Maidanak. The measurements were performed with the MASS instrument, a multi-aperture scintillation sensor that has been widely used for such studies in recent years at many observatories worldwide. Analysis of the data shows that the median seeing in the free atmosphere (at an altitude of 0.5 km and higher) is 0 ″46, while the isoplanatic angle is 2″.47. Given the large time constant (about 7 ms at good seeing), such conditions are favorable for using adaptive optics and interferometric measurements in the visible and near-infrared spectral ranges. 相似文献
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Hamid M. K. Al-Naimiy 《Astrophysics and Space Science》1986,118(1-2):51-56
Iraq is currently experiencing a praid cultural, scientific, and technical renaissance, and astronomy is a natural focus for the country's pride in the past achievements of the civilization which have flourished in Iraq. The current plans of the Space and Astronomy Research Center (SARC) include building a major observatory to work in the optical, IR and radio region of the spectrum.The core of the optical facility will be a 3.5 m optical telescope, together with 1.25 m telescope designed for efficient performance in the IR. These telescopes will be equipped with instruments for photographic, photometric and spectroscopic observations. A 30 m dish is also being built for millimeter/radio observations.SARC has selected an excellent observing site in the northern mountains of Iraq which has good seeing and clear dark skies. The sites selection was made with the collaboration of several leading astronomers and observatories from various countries.Paper presented at the IAU Third Asian-Pacific Regional Meeting, held in Kyoto, Japan, between 30 September–6 October, 1984 相似文献
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Douglas A. Simons Paola Amico Dietrich Baade Sam Barden Randall Campbell Gert Finger Kirk Gilmore Roland Gredel Paul Hickson Steve Howell Norbert Hubin Andreas Kaufer Ralf Kohley Philip MacQueen Sergej Markelov Mike Merrill Satoshi Miyazaki Hidehiko Nakaya Darragh O'Donoghue Tino Oliva Andrea Richichi Derrick Salmon Ricardo Schmidt Hongjun Su Simon Tulloch Maria Luisa García Vargas R. Mark Wagner Olivier Wiecha Binxun Ye 《Experimental Astronomy》2005,19(1-3):15-44
Results of a survey of instrumentation and detector systems, either currently deployed or planned for use at telescopes larger than 3.5 m, in ground based observatories world-wide, are presented. This survey revealed a number of instrumentation design trends at optical, near, and mid-infrared wavelengths. Some of the most prominent trends include the development of vastly larger optical detector systems (> 109 pixels) than anything built to date, and the frequent use of mosaics of near-infrared detectors – something that was quite rare only a decade ago in astronomy. Some future science applications for detectors are then explored, in an attempt to build a bridge between current detectors and what will be needed to support the research ambitions of astronomers in the future. 相似文献
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