观测的

The results of Venus observation with Danjon Astrolabe during 1983 at Shanghai Observatory are given in this paper.

1983年，上海天文台用丹容等高仪对太阳系中的白天观测目标——金星进行了试观测。

The bore-hole water temperature observation is a main earthquake precursor observation method of geothermal observation network .

井孔水温观测是地热观测网中主要的地震前兆观测方法。

Methods (1)We observed the serial sheet sections of the optic apex region obtained using collodion microtomy in 4 adult cadaver heads;(2)High resolution CT scanning and three dimensional images of the optic apex region were observed and measured in 10 adult volunteers;(3)High resolution magnetic resonance images of the optic apex region were obse.

①采用火棉胶切片技术对4例(8侧)成人眶尖区标本进行连续薄层断层解剖学观察；②使用高分辨力CT及三维重建技术观测10例(20侧)志愿者眶尖区；③观测5例(10侧)志愿者眶尖区高分辨力MRI断层扫描图像；④对30例(60侧)成人干颅骨标本和15例(30侧)成人湿性头颅标本的眶尖区结构进行显微解剖；⑤在手术显微镜和内窥镜下对3例成人头颅湿性标本模拟眶内经颅入路。

Especially,when there are local changes among the data,and a single parametric distribution family can\'t describe the observed data accurately,finite mixing distribution models usually make excellent performance.

特别是，当观测数据有局部变化，而单一的参数分布族无法确切地描述观测数据时，有限混合分布模型表现出色。

For planetary or double star observing, you'll want an eyepiece in at least the 150x range.

行星观测和双星观测，你将需要一个最少150倍的目镜。

The observation data during 1-31, August 2006 and the first guess from T213 numerical weather prediction system are used for analyzing the root mean square of observation error.

观测误差均方差分析使用2006年8月1-31日观测资料，国家气象中心T213L31全球中期分析预报系统的6小时预报作为背景场。

Kalman filtering is affected by the gross error that is inevitable in the observation of satellite.

卫星观测数据中不可避免地存在着粗差，一般的Kalman滤波易受观测粗差的影响。

In fractural physical model experiment, after the analysis of the reflected P wave varying with observed azimuth at a certain offset in the simulated fractured media, we get the traveltime difference varying with observed azimuth. Also we can infer the azimuthal NMO velocity difference in fractured media.

在裂缝物理模型实验中，通过对模拟的平行排列的垂直裂缝介质中反射纵波的固定偏移距随观测方位变化的结果分析，得出随观测方位变化的旅行时的差异，可以推出同样存在随观测方位变化的动校正速度的差异。

The transition radiation faculae on the rear side of a 20m thick target Ta was a smooth round structure with the center brighter than the periphery, indicating incoherent transition radiation and coherent transition radiation, which is close to the results of the theoretical simulations. For a 100m thick target Ta, the faculae was a star-structure and became smaller, which resembles a star-structure of the energetic proton emission. For a 10μm Ta+10m Cu+5m Ta composite target, the faculae was a ring structure and became bigger and non-uniform, looked like two apart faculae.

在厚度为20μm的Ta靶背表面观测到渡越辐射光斑呈现较平滑的圆形结构，而且中心亮度高于周围，这包含了非相干与相干渡越辐射的成分，与理论模拟结果接近；在厚度为100μm的Ta靶背表面观测到渡越辐射光斑呈现出星状结构，光斑较小，与高能质子发射出现的星状结构极其相似；在复合靶背表面观测到渡越辐射光斑虽然也呈现大致的圆形结构，但光斑较大，而且极不均匀，中间有很明显的光斑分裂。

5Ns. The peak position of N band emission as well as the distinct emission region slightly moves towards the open end of the cylindrical cavity, and this does not happen to O band emission. Radiation transport efficiency of 6% is obtained for the φ400×1200um cylindrical cavity heated by x-ray source with radiation temperature of 118 eV.

从时间分辨的X光强度轴向空间分布来看，在较长时间（约1～1.5ns）内，O带X光在整个观测缝对应的轴向范围之内均有较大的辐射强度，在X光强度空间分布的变化过程中，其强度峰值的空间位置基本不变；而对N带X光，则只在较短时间（约0.5ns）内，在整个观测缝对应的轴向范围之内可观测到X光辐射，但只在靠近输运源约300μm的范围内有较强发射，在柱腔末端600～700μm范围之内的辐射则很弱，N带X光辐射轴向空间分布曲线的峰值位置在朝柱腔末端的方向移动，移动量大约为130～250μm。

She gently rebuff ed him, but agreed that they could be friends

她婉言拒绝了，但同意作为朋友相处。

If in the penal farm, you were sure to be criticized.

要是在劳改农场，你等着挨绳子吧！