矿用随钻动态方位伽马仪器的研制与应用     

陈龙  陈刚  张冀冠 《煤田地质与勘探》2022,50(1):86-91

顺煤层瓦斯抽采钻孔是目前最直接最有效的瓦斯治理方法,自然伽马作为含煤地层识别常用的判识依据,可以根据地层放射性判断钻孔轨迹是否在目标层中。但现有的矿用伽马测井仪器只能进行滑动钻进测量,不适用于复合钻进及旋转导向钻进,无法满足伽马动态连续测量的工况。针对以上问题,在分析了煤矿井下随钻测量工况特点和伽马测井原理的基础上,通过低压直流载波双向通信技术进行孔底多扇区方位伽马数据的实时传输;采用屏蔽开窗的结构设计,实现单伽马晶体的8扇区分区测量;基于三轴MEMS加速度传感器和三轴MEMS陀螺仪不同的频率特性,采用互补滤波的动态测量方法,克服了回转钻进过程中振动和旋转对工具面向角测量的影响。通过地面性能测试和井下的工业性试验,验证了仪器在不同放射性地层分界面能正确反映出地层放射性变化规律。试验结果表明,仪器可以满足复合回转定向钻进时的地质导向测量要求,为煤矿井下顺煤层定向钻进提供了技术保障。   相似文献   

一种表示地球椭球体上椭圆的算法     

尹辉  谢玉波  李欣 《测绘科学》2009,34(5)

采用常规的投影算法表示地球椭球体上的椭圆时,所得椭圆与实际椭圆存在一定误差。针对上述问题,阐述了一种通过解算大地主题表示地球椭球体上椭圆的算法。通过几个实例,对两种算法进行了比较和分析,结果表明,通过解算大地主题表示地球椭球体上椭圆的算法具有非常高的精度。  相似文献   

GPS在地震仪器地理北方位定向中的应用     

张毅  顾春雷  王雷  徐如刚  李志平 《大地测量与地球动力学》2007,27(Z1):58-59

介绍了用GPS对台站数字化地震仪地理北方向的定位方法。试验表明,定向精度优于2′,完全满足地震仪器定向精度小于6′的要求。  相似文献   

A possible explanation of photon emission from supernova remnants by jitter radiation     

T. Ogasawara  T. Yoshida  S. Yanagita  T. Kifune 《Astrophysics and Space Science》2007,309(1-4):401-405

We investigate a possibility that non-thermal X-ray emission in a supernova remnant(SNR) is produced by jitter radiation, which is the analogue of synchrotron radiation in small-scale random magnetic fields. We can fit the multi-wavelength data of SNRs RX J1713.7-3946 (G347.3-0.5) and RX J0852.0-4622 (G266.6-1.2) by constructing pure jitter and inverse Compton (IC) emission models. We find that the physical fit parameters of random magnetic fields take values of several tens of μG strength and of the order of ∼10⁷ cm correlation length. These properties of random magnetic fields in collisionless shock of SNRs are discussed.   相似文献   

The drift model of “magnetars”     

I. F. Malov  G. Z. Machabeli 《Astrophysics and Space Science》2007,308(1-4):467-469

It is shown that the drift waves near the light cylinder can cause the modulation of emission with periods of order several seconds. These periods explain the intervals between successive pulses observed in AXPs, SGRs and radio pulsars with long periods. The model under consideration gives the possibility to calculate real rotation periods P of host neutron stars. It is shown that P≤1 s for the investigated objects. The magnetic fields at the surface of the neutron star are of order 10¹¹–10¹³ G and equal to the fields usual for the known radio pulsars.   相似文献   

区域Gamma混合模型的SAR图像分割   总被引：1，自引：0，他引：1  

李琴洁  杨学志  吴克伟  薛丽霞  郎文辉 《遥感学报》2014,18(5):1024-1033

针对传统Gamma混合模型用于SAR图像分割时忽略像素间空间相关性,导致分割结果不连续并产生大量误分割的现象,提出了区域Gamma混合模型的SAR图像分割算法。首先对图像进行分水岭分割,得到过分割区域块,然后将其作为输入样本进行基于Gamma混合模型的聚类,在模型的参数估计过程中进一步考虑区域间的空间相关性,设计邻域因子融入到迭代过程,得到邻域加权类分布概率。该算法充分利用像素间的空间相关性,能够降低噪声对分割结果的影响。通过合成图像和真实SAR图像的实验表明,本文算法能够实现SAR图像的准确分割。  相似文献   

Tail Emission from a Ring-like Jet: Its Application to Shallow Decays of Early Afterglows and GRB 050709     

Yuan-Chuan Zou  Zi-Gao Dai Department of Astronomy  Nanjing University  Nanjing   《中国天文和天体物理学报》2006,6(5)

Similar to the case of pulsars the magnetic axis and the spin axis of gamma-ray burst sources may not lie on the same line. This may cause the formation of a ring-like jet due to collimation of the processing magnetic axis. We analyze the tail emission from such a jet, and find that it has a shallow decay phase with a temporal index of -1/2 if the Lorentz factor of the ejecta is not very high, which is consistent with the shallow decay phase of some early X-ray afterglow detected by Swift. The ring-like jet has a tail cusp with sharp rising and very sharp decay. This effect can provide an explanation for the re-brightening and sharp decay of the X-ray afterglow of GRB 050709.  相似文献   

The sensitivity of EGRET to gamma-ray polarization     

John R. Mattox 《Experimental Astronomy》1991,2(2):75-84

A Monte Carlo simulation shows that the EGRET gamma-ray telescope aboard the GRO satellite does not have sufficient sensitivity to detect linear polarization, even for 100% polarized gamma-ray sources. This is confirmed by analysis of calibration data. Several data selection techniques suggested to enhance polarization sensitivity have been evaluated and found to not significantly improve sensitivity.NRC/NAS RESEARCH ASSOCIATE  相似文献   

低纬子午环绝对测定仪器瞬时方位差方法的改进(Ⅱ)     

彭青玉 《天文研究与技术》1997,(1)

在导出低纬子午环测定一颗星过卯酉、子午圈的记录时刻与瞬时方位差关系式的基础上，结合仪器在卯酉圈测定星对天顶距的方法［１］，提出了既可以绝对测定瞬时方位差，又可以绝对测定定位误差ε的新设想  相似文献   

A bivariate gamma distribution for use in multivariate flood frequency analysis     

Sheng Yue 《水文研究》2001,15(6):1033-1045

A gamma distribution is one of the most frequently selected distribution types for hydrological frequency analysis. The bivariate gamma distribution with gamma marginals may be useful for analysing multivariate hydrological events. This study investigates the applicability of a bivariate gamma model with five parameters for describing the joint probability behavior of multivariate flood events. The parameters are proposed to be estimated from the marginal distributions by the method of moments. The joint distribution, the conditional distribution, and the associated return periods are derived from marginals. The usefulness of the model is demonstrated by representing the joint probabilistic behaviour between correlated flood peak and flood volume and between correlated flood volume and flood duration in the Madawask River basin in the province of Quebec, Canada. Copyright © 2001 John Wiley & Sons, Ltd.  相似文献