震级特征图特点与a,b值关系

本文主要研究了a、b值的变化对震级特征图的影响。当a、b值的变化幅度不太大时,仍然可从震级特征图上识别出最小均匀震级等震级阈值;当a、b值的变化达到相当的幅度后,震级阈值点变模糊了。     

裂陷盆地洼槽演化规律研究——以歧口凹陷西部为例

裂陷盆地中洼槽的演化规律对烃灶的分布及生烃能力具有明显控制作用。歧口凹陷在古近纪经历了两期两向的裂陷活动,洼槽结构较为复杂,裂陷Ⅰ幕,在NW-SE向伸展作用下,形成了多个NE-NNE向洼槽;至裂陷Ⅱ幕,受N-S向伸展作用,NE-NNE向断层活动性逐渐减弱,NE-NNE向洼槽开始萎缩。本文基于控洼断层的空间组合样式及传播方式、洼槽内层序界面的接触关系,建立洼槽演化的3种模式;结合典型地震剖面、地层厚度图、控洼断层断距—距离曲线等相关证据,识别出歧口凹陷洼槽的演化规律。其中,歧南洼槽属于“生长连接型洼槽演化模式”,板桥洼槽属于“固定长度型洼槽演化模式”,而歧北洼槽属于“侧列叠覆型洼槽演化模式”。     

子宫肌瘤的CT诊断价值

本文回顾性分析了２１例经手术,病理证实的子宫肌瘤ＣＴ表现。指出子宫外形呈不规则结节样增大,边缘光整,强化后的混合密度征及边缘线影是ＣＴ诊断子宫特异性很强的征像。对那些多肌瘤,瘤体较大,合并复杂变性者,能弥补Ｂ超因肠道气体等多种因素所致的不足。因此ＣＴ在子宫肌瘤的影像上有重要价值。     

云南地区地震短临预报实践

１９９７年４－６月云南省地震局对滇西南重点监视区做了短临预报,但这期间未发生所预期的地震。而滇西南地区６级地震的背景和省内的前兆异常变化是明显的。为此,认为前兆异常是区域应力场增强的结果。异常与地震是相互伴生的兄弟关系,不是父子间因果关系,是造成地震虚报的主要原因。     

平行走滑断层相互作用的粘弹模型和减震作用

研究了二维粘弹性介质中平行走滑断层的相互力学作用及其地震活动性的影响。当一条断层发生滑动,将导致平行断层面上剪切应力减小,因此,可能推迟平行断层发生滑动,推迟时间在几年至几百年的范围内,这取决于发生滑动的断层与平行断层之间的距离,以及平行断层自身应力积累孕育地震过程经历的时间。     

基于地基微波辐射计资料对成都双流机场两次雷雨过程的分析

利用地基微波辐射计资料,比较了2017年7月成都双流机场的两次雷雨过程,根据天气形势分为"两高切变"和"东高西低"2类,在此基础上分析微波辐射计要素变化特征,结果表明:在垂直方向0～10 km,以相对湿度达到80%来区分干区和湿区,则两次过程前3 h,相对湿度在垂直方向均呈现"上下干、中间湿"三层结构,并早于近地层前2 h达到饱和状态;过程期间相对湿度呈现"上干、下湿"两层结构;过程结束后湿层抬高,低层变干。两次过程水汽含量充沛,保持在70 kg/m~2以上,峰值超过85 kg/m~2。每一次中阵雨发生后水汽含量都会短暂回落,但仍高于过程前的数值,不足2 h后再次发生中阵雨。由0℃线高度变化可知,降水过程中,暖区(温度≥0℃)内相对湿度≥90%;云中液态水含量主要分布于6 km以下,温度在0℃以上的液态水占比很高,故两次过程以暖云降水为主。雷雨前1 h左右有"低层气温上升,0℃层抬升,K指数、CAPE指数也明显增大"的典型特征。降水发生在相对湿度、水汽总含量、云中液态水含量和稳定度指数快速增长的波峰中。     

我国电子政务建设的机遇挑战及其对策

通过对电子政务发展战略的深入分析 ,指出我国电子政务的建设正面临四个挑战 ,包括重复建设、无序操作、忽视应用、管理滞后等。面对重复建设、建设无序、忽视应用、管理滞后等问题 ,提出了迎接四个挑战的具体对策     

Study on a gravity precursor mode of the <Emphasis Type="Italic">M</Emphasis><Subscript>s</Subscript>=7.0 Lijiang earthquake

To study the seismogeny process or the precursory behavior of the 1976 M _S=7.0 Lijiang earthquake, we analyze the repeat gravity data with high precision from the Western Yunnan Earthquake Prediction Experiment Area (WYEPEA) and the related results of geology and geophysics survey in this paper. Considering the gross errors caused by observation data and model difference, we have firstly inverted the slip distribution of the main active faults with time based on the robust Bayesian least squares estimation and multi-fault dislocation model. The results show that the slip changes of the faults with time from 1990 to 1997 obviously reflect the preparation process of the Lijiang earthquake. The images of main precursor mode have the characteristic of main shock-after shock type, which is agreement to the model of coupling movement between crust density and crust deformation (DD mode of coupling movement).     

The Generating Region of Bidirectional Electron Beams in the Corona

Metric and decimetric type III bursts and microwave spike emissions with negative and positive frequency drift rates which were observed with radio spectrometers at Yunnan and Beijing Observatories are presented. The frequencies and heights at which the bidirectional electron beams originated are estimated. Three events reveal a separatrix frequency (at 250, 1300, and 2900 MHz) between normal- and reverse-drifting radio bursts, indicating a compact acceleration source where electron beams are injected in both upward and downward directions. These cases may indicate that the changeover frequencies of bidirectional electron beams are within a large band from 250 to 2900 MHz and the frequency bands of separatrices are in very small (4 to 100 MHz) and different bands. These type III bursts appear to be a plasma emission phenomenon from a beam of electrons which seem to have widely separated acceleration regions from the high to the low corona. These cases suggest that current sheets that separate open and closed magnetic fluxes in the low corona, and oppositely directed open field lines in the high corona are possible sites for bidirectional electron acceleration. The regions of magnetic topology from closed to open magnetic field structures should be very large (from about 20000 to 107000 km above the photosphere).     

Type III burst pair

We present a special solar radio burst detected on 5 January 1994 using the multi-channel (50) spectrometer (1.0–2.0 GHz) of the Beijing Astronomical Observatory (BAO). Sadly, the whole event could not be recorded since it had a broader bandwidth than the limit range of the instrument. The important part was obtained, however. The event is composed of a normal drift type III burst on the lower frequency side and a reverse drift type III burst appearing almost simultaneously on the high side. We call the burst type III a burst pair. It is a typical characteristic of two type III bursts that they are morphologically symmetric about some frequency from 1.64 GHz to 1.78 GHz on the dynamic spectra records, which indicates that there are two different electron beams from the same acceleration region travelling simultaneously in opposite directions (upward and downward). A magnetic reconnection mode is a nice interpretation of type III burst pair since the plasma beta 0.01 is much less than 1 and the beams have velocity of about 1.07×10⁸ cm s^–1 after leaving the reconnection region if we assume that the ambient magnetic field strength is about 100 G.