软土层施工桩基的新方法滚压法

介绍软土层用新型孔底工具－滚压器施工桩基的工作原理、施工工艺,滚压器基本结构及不同直径滚压器的技术特征。     

低周反复荷载作用下复合耗能支撑钢筋混凝土框架结构的抗震性能试验研究

本文介绍了三榀钢支撑钢筋混凝土框架结构（包括两榀复合耗能支撑框架、一榀普通支撑框架）在低周反复荷载作用下的试验结果。对复合耗能支撑框架结构在低周反复荷载作用下的工作性能（包括受力性能、破坏形态、滞回曲线、骨架曲线、延性和耗能能力等）进行了探讨,揭示了复合耗能支撑框架结构良好的抗震性能。     

新型耗能(阻尼)减震器的开发与研究

本文阐述了耗能减震的概念和原理,提出了耗能减震器设计的新思想,研制开发了多种新型实用耗能（阻尼）减震器,并对其中的圆环耗能器、双环耗能器、架颈圆环耗能器、弹塑性－摩擦复合耗能器等进行了循环荷载试验,考察了耗能器代作性能和耗能性能,对已装与未装耗能减震器的钢筋混凝土框架模型进行了伪动力对比实验,进一步考察了耗能减震器的减震效果。在试验研究的基础上,地耗能（阻尼）减震结构体系的分析方法进行了研究,并编     

双刚臂位移计及误差标定

在断层活动的监测中或有关地震规律的研究实验中多需测量位移,为便于连续监测和自动记录常用贴有应变片的弹簧片做位移计(图1)。设△为所测位移,ε为弹簧片表面纤维的最大应变,则此类位移计的线性特性用△/ε表示。对于这种常用位移计来说     

滑翔与气流

无摩托之飞机的飞行——滑翔,在十九世纪的末叶已经有人试验过,但是在1896年首创此种飞行的德人Lilienthal殉难後,继续作此种尝试的人很少,而同时有摩托之飞机的发展甚速,1911至1912年德国Darmstadt的学生曾在Rhon山中作滑翔训练,Hans Guteimuth造     

室外大池马氏珠母贝育苗试验

本试验利用一个室外露天水容量为187立方米的水泥池进行马氏珠母贝人工育苗,一次育出贝苗5065万只,平均每立方米水体收贝苗27.08万只。室外大池育苗具有耗饵量少,节约人力,培育的幼虫和贝苗生长快和产苗量大等优点,能够迅速提高贝苗总产量,解决目前存在的贝苗(?)足的困难,值得提倡推广。     

Infrared Characteristics of Associated Sources of Water Masers

We present an analysis of the infrared properties of 1417 water masers collected from the literature published by December 2004. The associated infrared sources of the water masers were identified with IRAS and MSX (Midcourse Space Experiment) catalogues. There are 1252 water masers associated with IRAS sources within 1', which include 700 interstellar and 552 stellar sources. For 382 sources, the IRAS counterpart identification and the maser classification are new. We found the colors of the interstellar maser sources are much redder than those of the stellar ones at IRAS wavelength bands; 99% of the interstellar maser sources are above black body line, while 95% of the stellar masers are below. The distribution difference of the two kinds of masers shown in the color-color diagram is due to their different optical depths and temperature distributions of dust regions. There are 743 water masers with MSX counterparts, of which 552 are interstellar masers and 191 are stellar masers. MSX colors of the associated sources of water masers are here analyzed for the first time. The color differences among the MSX bands are small and the interstellar masers are redder than the stellar masers. There is a correlation between the intensity of the stellar water maser emission and that of the 12μm and 25μm emissions, while there is no correlation between the water maser emission and the 8 μm emission. The infrared intensity increases with increasing wavelength for the interstellar masers, while it is the opposite for stellar masers. These results may provide clues for the pumping of water maser and for the properties of the two kinds of maser emission regions.