1.Near the church is Sheshan astronomical observatory which has been changed into an astronomical museum.
这里曾经两次观测到哈累彗星，一个相当了不起的记录。
2.Complex type III-moving IV solar radio burst on Sep. 23, 1998 observed with radio spectrometers (1 - 2 GHz and 2.6 - 3.8 GHz) at Beijing Astronomical Observatory (BAO) is analyzed preliminarily, combining with the data obtained from the SSRT (5.7 GHz ) in Russia and radio spectrometer in Germany. These study fields of electron acceleration and magnetic structures in the corona are expanded.
利用北京天文台1998.09.23日1—2 GHz和2.6-3.8 GHz频谱仪观测到的一个III—IV型复杂大爆发,结合俄罗斯SSRT和德国分米-米波动态频谱仪的观测资料,进行了初步的比对分析,拓展了关于日冕电子加速和日冕磁结构方面的一些研究内容.
3.The CCD observation of 2237+0305 using the 1-m reflector of Yunnan Astronomical Observatory gives the surface intensity profiles of this system. Detailed analysis shows that the angular distance between the QSO and the center of the spiral galaxy is less than 0.1″.
本文利用云台1米望远镜及CCD系统对2237+0305进行观测,给出等光强度分布,分析表明,旋涡星系中心与类星体的角距小于0.1角秒。
4.Although it is not clear who built the monument, nor for what purpose, it has been speculated that it was either a temple dedicated to the worship of ancient earth deities, an astronomical observatory or a sacred burial site.
人们至今还不清楚，究竟是谁建造了这一奇特古迹，为什么建造了这一古迹，但人们推测，巨石阵要么是庙宇，要么是天文台，或者是神秘墓地。
5.High Energy Astronomical Observatory
高能天文台
6.Based on ACRS represented by the Hipparcos Catalogue, the positions and absolute proper motions of 264 stars in a 70′×70′ region around the globular cluster M13 are reduced by plates taken with the 40cm refractor at Sheshan station of Shanghai Astronomical Observatory, referred to the positions and absolute proper motions in the Hipparcos (for 5 stars) and Tycho-2 (for 38 stars) Catalogues. The membership probabilities of these stars are estimated.
以《Hipparcos星表》体现的国际天球参考架为基础 ,对球状星团M13中心附近 70′× 70′天区内2 64颗恒星 ,使用上海天文台佘山口径 4 0cm双筒折射望远镜拍摄的底片资料 ,以 5颗《Hipparcos星表》中恒星和 38颗《Tycho - 2星表》中恒星的位置和绝对自行为参考 ,归算得到了位置和绝对自行 ,并估计了成员概率。
7.On the basis of the JPL and GFZ standard inverse algorithm of neutral atmospheric by GPS occultation data, a computation process of neutral atmospheric retrieval in Shanghai Astronomical Observatory (SHAO) was developed.
结合JPL和GFZ的中性大气标准反演算法,发展了上海天文台中性大气掩星标 准反演算法流程.
8.e identified the night sky emission lines from 5300 to 8200 Angstrom at XinglongStation, Beijing Astronomical Observatory, and measured the variations of airglow emissionlines during one night.
介绍了夜天光光谱的观测方法，给出了北京天文台兴隆观测站530nm－820nm的夜天光发射光谱，并对它们进行了证认，测定了大气辉光线的夜变化；
9.Their mission was to reach Tahiti before June 1769, establish themselves among the islanders, and construct an astronomical observatory.
他们的任务是在1769年6月前抵达塔西提岛，融入当地岛民中，建立天文观测站。
10.Active region 5229 was studied during 13-18 November 1988 using Hβ filergrams and PeI 5324 Viedomagenetograms acquired at Huairou Solar Observing Station of Beijing Astronomical Observatory.
本文研究了活动区5229中的H_β耀斑和磁场的关系。 所用资料为北京天文台怀柔太阳观测站1988年11月13—18日期间获得的(时值活动区5229位于E40°W40°)。
