CDJ-1型超声波大口径桩孔检测仪使用中的几个问题

ＣＤＪ１型超声波大口径桩孔检测仪是专为检测工程基桩孔和地下连续（防渗）墙而研制的。几年来,在国家重点建设工程和其它基础工程中得到了应用,对提高工程桩孔（连续墙槽）的施工质量起到了重要的监督和促进作用。因为是新型仪器,有些单位及操作者在使用中遇到一些问...     

大口径气举反循环钻具提效74%

正日前,由河南省煤田局承担的河南省国土资源厅科技攻关项目"大口径气举反循环钻具研制及应用研究"通过审查验收。项目研制了直径219.1/168.3毫米螺纹联接双壁钻杆、直径168.3毫米内平单壁钻杆、气举反循环水龙头、双壁主动钻杆及反循环钻头等配套器具,经生产性试验证明:该套组合钻具强度高、密封性能好、连接形式独特,可满足直径600毫米~1500毫米的大直径工程井气举反循环钻井施工,在同等技术条件下,比正循环钻进效     

CIPP拉入内衬修复技术在大口径排水管道上的应用

如何快捷、简便、经济、有效地修复大口径排水管道病害,使管道系统保持在较好的工作状态,已成为市政管网安全运行的重要课题之一,天津开发区在泰丰路DN1500污水管道上成功运用CIPP浸渍玻璃纤维拉入法修复技术,是国内管道修复技术应用的突破,对今后全国运用CIPP技术对遭到腐蚀或结构性破坏的大口径管道进行修复,延长管道的使用寿命,起到了示范作用。     

大口径顶管技术在水利引水工程中的应用

本文通过大口径顶管技术在水利引水工程中的应用案例,介绍了非开挖顶管技术在设计方案选择中的优越性以及施工中关键技术数据的计算方法。     

深孔及松软地层大口径绳索取心钻具的研究与应用

为解决深孔大口径及松软地层取心难的问题,推进取心钻探技术的发展,研发了一套大口径绳索取心钻具。着重介绍了大口径绳索取心钻具的结构特点、技术参数、技术创新及使用效果。应用结果表明,该大口径绳索取心钻具结构合理、各机构动作可靠、岩心采取率高,能够满足深孔及松软地层的取心要求。     

GYD-20型全液压动力头工程钻机的研制

针对传统工程钻机生产制造周期长、自动化程度低、劳动强度大、施工效率低等弊端,研制了GYD-20型全液压动力头工程钻机。介绍了该钻机的结构特点及其应用于大口径基础桩孔、煤矿通风孔钻进的情况和效果。     

大口径瓦斯抽排井施工扩孔分级设计优选探讨

受现有钻探设备能力限制,大口径瓦斯抽排井工程通常采用“先导钻进+分级扩孔”施工方法。通过扩孔所需回转扭矩的计算分析,对常用大口径瓦斯抽排井扩孔分级的设计进行了探讨。     

金华山煤矿大口径瓦斯抽排孔施工技术

为了减少煤矿瓦斯的危害以及对其综合利用,国家鼓励并大力支持大口径瓦斯抽排孔项目的建设。陕西铜川金华山煤矿一口大口径瓦斯抽排孔,孔径850 mm,终孔深度401.6 m。从钻进方法、钻具级配、钻进技术参数、冲洗液、圆孔、溜孔、井底护管安装固结、充填循环泥浆、下管、固管、透孔放水等方面详细地介绍了大口径瓦斯抽排孔小径透巷后的特殊施工工艺和相关的技术措施。     

观测场照明电路造成自动站温度异常故障分析

1引言 到目前为止,吉林省已经建成投入使用的Ⅰ型自动气象站（以下简称自动站）有5个,Ⅱ型自动站有51个,为提高天气预报准确率和气象服务时效性奠定了坚实的基础。自动站正常工作,做好技术保障是非常重要的。本文讨论一起DYYZ-Ⅱ型自动站由于观测场照明电路引起温度数据异常的处理方法,供自动站维修人员参考。     

Study of white-light flares observed by Hinode

White-light flares are considered to be the most energetic flaring events that are observable in the optical broad-band continuum of the solar spectrum. They have not been commonly observed. Observations of white-light flares with sub-arcsecond resolution have been very rare. The continuous high resolution observations of Hinode provide a unique opportunity to systematically study the white-light flares with a spatial resolution around 0.2 arcsec. We surveyed all the flares above GOES magnitude C5.0 since the launch of Hinode in 2006 October. 13 of these kinds of flares were covered by the Hinode G-band observations. We analyzed the peak contrasts and equivalent areas (calculated via integrated excess emission contrast) of these flares as a function of the GOES X-ray flux, and found that the cut-off visibility is likely around M1 flares under the observing limit of Hinode. Many other observational and physical factors should affect the visibility of white-light flares; as the observing conditions are improved, smaller flares are likely to have detectable white-light emissions. We are cautious that this limiting visibility is an overestimate, because G-band observations contain emissions from the upper atmosphere.Among the 13 events analyzed, only the M8.7 flare of 2007 June 4 had near-simultaneous observations in both the G-band and the blue continuum. The blue continuum had a peak contrast of 94% vs. 175% in G-band for this event. The equivalent area in the blue continuum is an order of magnitude lower than that in the G-band. Very recently, Jess et al.studied a C2.0 flare with a peak contrast of 300% in the blue continuum. Compared to the events presented in this letter, that event is probably an unusual white-light flare: a very small kernel with a large contrast that can be detected in high resolution observations.