共查询到17条相似文献,搜索用时 360 毫秒
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较详细地讲述了云南天文台三孔较差宁度监视仪的情况,然而,与一般天文理论和天文技术的专题研究不一样,天文仪器的研制有如说是研究,还不如说是归纳;它不是分析一个具体的沿示解决的难题,而是把许多已知的理论和技术综合起来,构成一台具体的仪器。所以,本文把许多至少是表面上互不相关的理论和技术问题归纳到一篇论文中。仪器是有许多模块组成的,为了起来逻辑性较强,我们将仪器分模块叙述,全文遵循如下顺序: 相似文献
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云南天文台丽江高美古和昆明的大气视宁度研究 总被引:5,自引:1,他引:4
研究云南天文台昆明凤凰山和丽江高美古两地点的大气视宁度。利用云南天文台于1994年建立的3孔较差视宁度监视仪(3孔DIMM),对这两个地点的视宁度对比观测。还利用云南天文台的1米望远镜所得到的视宁度与3孔DIMM所测的视宁度进行对比。1米望远镜和3孔DIMM同时观测了7个晚上,各取得308组数据,它们的视宁度平均分别为0.90〃和0.84〃。还讨论了3孔DIMM采用不同曝光时间对视宁度测量值的影响,从实验得出3孔DIMM采用20ms曝光比采用8ms曝光所测视宁度的值要好15%左右。从1995年5月-1996年12月,对丽江高美古和昆明凤凰山二地进行了视宁度的对比观测。在高美古和昆明分别观测了234夜和256夜,观测结果是两个点的视宁度平均;丽江为0.70〃,昆明为0.95〃,同时也统计了两个点的月平均视宁度和最好夜的视宁度,并讨论了两地视宁度随时间的变化规律。 相似文献
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从天文选址的角度出发 ,介绍了影响望远镜光学成像质量的大气湍流的成因、特性以及它对星光波前的影响 ,进而对衡量大气宁静度的量度值———大气视宁度做了详细的叙述 ,包括其测量方法 ,以及目前国际天文选址界常用的较差像运动测量仪的测量原理 ,介绍了云台三孔较差像运动测量仪的光学和硬件结构组成部分 ,对图像处理 /采集软件中用Waldie法计算大气视宁度值与用Roddier法计算大气视宁度值的不同之处进行了理论的分析 ,编写了Roddier法相应软件 ,并用于实测中测量了大气视宁度的值 ,得到一些有意义的结果。 相似文献
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Youssef Hach Abdelouahed Abahamid Mohammed Sabil Abdelmajid Benhida Zouhair Benkhaldoun Abdelfatah Habib Youssef Elazhari 《Experimental Astronomy》2010,28(2-3):87-99
Over the past years, several differential image motion monitors (DIMM) have been built almost everywhere. The DIMM instrument is made up of simple material such as telescope, mask, camera ..., and it is widely used in seeing measurement campaigns. In order to carry out a prospecting campaign, for the European Extremely Large Telescope (ELT) project, in the Moroccan High Atlas, we have built a new DIMM instrument in our laboratory. To characterize this instrument, we have carried out a cross-calibration between DIMM monitors using different configurations. In this paper we will present the results of those various experiments respectively at Oukaimden site and at the “École Normal Supérieure” (ENS) in the city of Marrakech. 相似文献
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A. Ziad R. Gredel J. Aceituno J. Borgnino F. Hoyo A. Irbah F. Martin U. Thiele S. Pedraz 《Monthly notices of the Royal Astronomical Society》2005,362(2):455-459
The main atmospheric optical parameters have been measured at the Calar Alto Observatory simultaneously using the Generalized Seeing Monitor (GSM) and a Differential Image Motion Monitor (DIMM) during several nights in 2002 May. The temporal evolution of the seeing, the outer scale, the isoplanatic angle and the coherence time have been analysed. There is excellent agreement between the seeing measurements provided by the two instruments, particularly when the turbulence is slow. Indeed, the GSM measurements are corrected from the exposure time when the DIMM data were recorded for at least 5 ms. From almost three years of DIMM (at 5 m height above ground) data, a seeing of 0.92 arcsec with a standard deviation of 0.31 arcsec has been obtained for this site. The outer scale , the isoplanatic angle θ0 and the coherence time τ0 measured with the GSM are well fitted with log-normal distributions with median values of 22.9 m, 2.27 arcsec and 3.7 ms, respectively. 相似文献
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总结和综述了云南天文台20年来在太阳光学仪器研制和改造,太阳活动现象观测研究,太阳活动预报和国际交流合作方面的成果和进展。 相似文献