地震地球物理数据监控软件设计与实现     

陈凯  易江  孙国栋  于天航  汪建 《地震地磁观测与研究》2021,42(3):291-297

台站设备故障响应和风险排除是地震监测工作的基本内容,针对其便捷性和高时效性要求,采用Java语言,开发基于Android平台的地震地球物理数据监控软件。该软件整合重庆市地震局监测工作中的各项业务需求,采用云服务、Tomcat服务器及百度地图等技术,实现了数据实时查看及历史数据波形浏览等功能,及时获取仪器设备工作状态,及时发现设备故障并进行维护,工作效率得以提高。  相似文献   

基于1973年炉霍MS7.6地震震后跨断层变形的地震轮回特征     

杜方  吴江  梁明剑 《地震地磁观测与研究》2021,42(z1):131-135

1 研究背景 地震活动断层不同区段和时段均具有不同的力学特性,主要是表现在活动断层上发生地震的断层段所呈现的震前、同震、震后和震间4个时域范围内的滑动行为.换言之,地震活动断层的滑动行为分为震前、同震、震后和震间4个滑动阶段.通过研究活动断层地震破裂段震前、同震、震后和震间滑动,可深入破解沿活动断层破裂段的应力、应变的积累和释放的时空信息变化(Reilinger et al,1999;Yagi et al,2001;Ozawa et al,2004).  相似文献   

关于促进国内气象企业健康发展的思考     

王柏林  姜长波  刘欣  刘新伟  黄秋菊 《气象科学进展》2022,(1):37-43

经济全球化和服务贸易市场化趋势的加快,特别是新媒体技术和信息技术的快速发展,为我国气象服务发展带来了良好机遇和严峻挑战.进入新时代,我国气象企业迈入快速发展的重要机遇期.2015—2016年,中国气象局适应气象服务体制改革,逐步开放气象信息服务市场、鼓励社会企业参与气象仪器研发生产、规范防雷检测资质管理,培育气象服务市...  相似文献   

物质点强度折减法边坡失稳判据选择方法     

蒋先平  张鹏  卢艺伟  刘磊磊  张明辉 《地质科技情报》2022,41(2):113-122

用物质点强度折减法求解边坡安全系数时,需要选择一定的失稳判据,而采用不同的失稳判据获得的安全系数通常存在一定差异.为此,采用物质点强度折减法对两个边坡算例进行了稳定性分析,对比研究了文献中常用的4种边坡失稳判据(计算不收敛、特征点位移突变、塑性应变贯通及界限值判据)在计算边坡安全系数时的合理性及适用性.同时,将Spen...  相似文献   

俯冲带板内地震竖向加速度谱阻尼修正系数模型研究   总被引：1，自引：0，他引：1       下载免费PDF全文

陈心锋  姜妍旭  刘名吉 《地震学报》2022,44(2):339-355

基于日本K-NET和KiK-net台网的4695条俯冲带板内地震记录,采用最小二乘法对阻尼修正系数(DMF)的几何均值进行关于阻尼比和谱周期的回归拟合,分场地类别建立了考虑阻尼比和谱周期的竖向加速度谱DMF模型.为探究震源、路径和场地效应对该模型残差分布的影响,采用随机效应模型将残差分离得到各类残差及相应的残差标准差,...  相似文献   

基于Web Services和.NET技术的新一代Web GIS研究与开发   总被引：38，自引：2，他引：36  

朱江  宋关福  钟耳顺  张继南  李伟顾  胡中南 《地理信息世界》2004,2(2):17-20

分析了当前主流Web GIS中普遍存在的问题,并基于Web Service和．NET技术。提出了新一代的网络地理信息系统技术框架——面向服务的Web GIS软件平台框架,该框架体现了“服务即是软件,软件即是服务”的全新理念。最后介绍了基于Web Service和．NET技术的新一代Web GIS平台——SuperMap IS．NET的设计与实现。  相似文献   

On the Systematic Errors in the Astrometric Catalogues ACR and CMC13 Based on CCD Drift Scanning Observations     

Li-ping Jiang   《Chinese Astronomy and Astrophysics》2008,32(2):216-228

Error analyses are made of ACR (Astrometric Calibration Regions along the celestial equator) and CMC13 (Carlsberg Meridian Catalogue 13), two astrometric catalogues compiled on the basis of CCD drift scanning observations and published respectively before and after 2000. Through a comparison with the UCAC2 (the second U.S. Naval Observatory CCD Astrograph Catalogue), the form and size of the errors are analyzed numerically. The main and possible sources of the errors are analyzed from the standpoint of observing mode and data reduction. It is found that there is evident magnitude difference between the ACR and CMC13 in the equatorial direction, and that there exists periodic variation close to the CCD field of view along the right ascension and also a systematic variation close to the size of reduction zone along the declination.  相似文献   

Variability Study of the SX Phoenicis Star BL Camelopardalis     

Jian-Ning Fu  Chao Zhang  Kanokwan Marak  Chayan Boonyarak  Pongsak Khokhuntod  Shi-Yang Jiang 《中国天文和天体物理学报》2008,8(2):237-244

New time-series photometric observations of BL Cam in the V band and white light were made during 2005 to 2007 at the Xinglong Station of China. The frequency analysis confirms two closely separated frequencies, 25.181 d-1 and 25.571 d-1, but the frequency of 31-32 d-1 reported in the literature was not detected in the new data. New times of maximum light were determined from both our light curves and those available on Internet, allowing a more comprehensive study of the O - C diagram, together with the times of maximum light in the literature. A new interpretation, including the period increasing before 1988 and decreasing since 1992 of BL Cam and the light-time effect in a binary system, looks plausible.  相似文献   

Formation of Transient Coronal Holes during the Eruption of a Quiescent Filament and its Overlying Sigmoid     

Li-Heng Yang  Yun-Chun Jiang  Dong-Bai Ren 《中国天文和天体物理学报》2008,8(3):329-336

By using Hα, He I 10830, EUV and soft X-ray (SXR) data, we examined a filament eruption that occurred on a quiet-sun region near the center of the solar disk on 2006 January 12, which disturbed a sigmoid overlying the filament channel observed by the GOES-12 SXR Imager (SXI), and led to the eruption of the sigmoid. The event was associated with a partial halo coronal mass ejection (CME) observed by the Large Angle and Spectrometric Coronagraphs (LASCO) on board the Solar and Heliospheric Observatory (SOHO), and resulted in the formation of two flare-like ribbons, post-eruption coronal loops, and two transient coronal holes (TCHs), but there were no significantly recorded GOES or Hα flares corresponding to the eruption. The two TCHs were dominated by opposite magnetic polarities and were located on the two ends of the eruptive sigmoid. They showed similar locations and shapes in He Ⅰ 10830, EUV and SXR observations. During the early eruption phase, brightenings first appeared on the locations of the two subsequent TCHs, which could be clearly identified on He Ⅰ 10830, EUV and SXR images. This eruption could be explained by the magnetic flux rope model, and the two TCHs were likely to be the feet of the flux rope.  相似文献   

旅游地生命周期曲线模拟的初步研究--Logistic曲线模型方法的应用   总被引：18，自引：0，他引：18  

吴江  黄震方 《地理与地理信息科学》2004,20(5):91-94

旅游地生命周期理论已经提出了很多年,这一理论的研究仍然在发展,尤其是对旅游地生命周期曲线的模拟做过很多有益的尝试。该文运用Logistic曲线对旅游地生命周期的发展阶段进行模拟,并应用Stella Ⅱ语言建立了模型,代入一定的数据进行处理,模拟旅游产品生命周期曲线,对这一曲线的主要影响因素进行了讨论。得出旅游市场预测的非线性规律,并讨论回头客对旅游地持续发展的重要性。  相似文献