Determination of Event Magnitudes With Correlated Data and Censoring: A Maximum Likelihood Approach     

K. L. Mclaughlin  R. H. Shumway†  T. W. Mcelfresh† 《Geophysical Journal International》1988,95(1):31-44

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2020年前我国核能发展的策略和目标研究     

潘自强  沈文权 《铀矿地质》2004,20(5):257-259

本文提出了我国核电发展的 4项策略 ,明确了近中远兼顾的 3个层次的发展目标及相关的重点工程。  相似文献   

Nuclear modification factor for quarkonium production in high energy proton-nucleus collisions within the parton saturation approach     

Érison S. Rocha  Magno V. T. Machado 《Astronomische Nachrichten》2024,345(2-3):e230165

In this work, we analyze nuclear effects in the inclusive production of quarkonium in proton-nucleus collisions at high energy regime. A theoretical framework that includes initial state effects like nuclear shadowing and gluon density saturation is considered. Numerical results for nuclear modification factor, $R_{pA}(y)$, as a function of meson rapidity in proton-nucleus collisions are presented. The parameter-free predictions are compared to the available data from the Large Hadron Collider. Discussion on the main theoretical uncertainties is made, with emphasis on the phenomenological models for the nuclear saturation scale.  相似文献   

影响靖宇地区温带气旋的统计分析     

蔡秀华  陈辉  曹鸿兴  吕文忠 《气象》2009,35(12):83-87

核电站因它不排放如二氧化碳这样的温室气体,核电对降低能源部门的碳密集作出了贡献,因此愈益受到人们的重视.在对核电站地区的天气、气候环境进行分析的基础上,对影响靖宇核电站地区的温带气旋作了研究.结果表明:1949-2007年期间影响靖宇地区的温带气旋计111个;受温带气旋影响的年数有41年(约2/3).影响靖宇地区且产生强降雨的温带气旋,主要发生在6、7、8月这3个月,并且一半以上出现在7月.影响靖宇地区的温带气旋大部分是东北气旋,占总数的65%;蒙古气旋与华北气旋次之.此外,对造成严重影响的温带气旋的个例也从天气学角度进行了分析.  相似文献   

基于RAMS/CFORS Ⅱ模式一次低空核试验放射性烟云扩散的数值模拟     

张彦  郑毅  王自发 《气候与环境研究》2008,13(6)

采用RAMS／CFORS Ⅱ模式模拟了一次低空核试验烟云的传输和沉降过程。CFORS Ⅱ模式是在RAMS／CFORS模式的基础上开发的,可用于对核试验放射性烟云长距离输送和沉降过程的模拟研究。模拟表明：对流层中低层的低压槽系统对本次低空核试验烟云的水平传输和垂直扩散起着重要的影响作用;烟云的长距离传输速度呈现出随高度递减而减小的趋势,在6000m以上,烟云在爆后48h即东移入海,6000m以下,烟云在中国大陆的扩散和沉降维持了5d以上;爆后2天内以大粒子沉降为主,其后以小粒子沉降为主,小粒子的放射性远小于大粒子,在爆后第4天,放射性沉降就减小了3个量级,而小粒子的沉降范围是大粒子的5倍以上。通过模拟和观测对比表明,模拟结果基本符合实际烟云的传输和沉降态势。  相似文献   

The Origin of the Element Eu in Extremely Metal-poor Halo Stars     

Jun-an Dai  Qiu-he Peng 《Chinese Astronomy and Astrophysics》2009

The fast neutron capture process (the r-process) occurs in the neutron-rich circumstance. However its concrete physical environment is not very clear. With recent progress in observations, many extremely metal-poor halo stars have been discovered. They have two characteristics: one is the overabundance of fast neutron elements with the relative abundance consistent with that of the sun; the other is that fast neutron element contents in stars at the same metal abundance have a very large dispersion. This provides a particular way to study the origin of the r-process. Simulation was used to study the galaxy's evolution process and the resulting dispersion of fast neutron nuclide contents in stars. The model of galaxy evolution obtained in this way not only contains spontaneous star formation in the gas region, but also includes the star formation excited by the supernova explosion. It is shown from our results that the supernovae at the low mass end should be the place producing the fast neutron nuclides. In addition, it is also shown that the non-uniformity of the galaxy evolution caused by the supernova explosion is not enough to explain the observed dispersion of fast neutron element contents in halo stars. This problem should be further studied.  相似文献   

Study of the dependence of the star formation rate in the nuclear regions of 39 Kazarian galaxies on their integral parameters     

V. Zh. Adibekyan  A. R. Petrosian 《Astrophysics》2009,52(2):192-204

A statistical study of the dependence of the star formation rate in the nuclear regions of 39 Kazarian galaxies on the integral parameters of these galaxies is carried out on the basis of spectra from SDSS DR6. The value of SFR/kpc² for our sample lies in the range 0.013÷2.04M _⨀ year⁻¹kpc⁻² (with the maximum value of 2.04 corresponding to the Kaz 98 (merger)). It is found that the surface density of the rate of star formation correlates positively with the bar structure parameter and EW(Hα), and that, for spiral galaxies of early morphological types, SFR/kpc² is greater than for the later types. It is shown that the color B-R for the galaxies and the color (u − g) _nucl for the nuclear region correlate positively with the total absorption A(Hα) in the Ha line for the nuclear region. The average value of A(Hα) for our samples is found to be A(Hα)=1.3±0.09 magnitudes. Translated from Astrofizika, Vol. 52, No. 2, pp. 211–224 (May 2009).  相似文献   

The approximation of neutrino heat conduction with neutrino scattering     

A. V. Yudin  D. K. Nadyozhin 《Astronomy Letters》2008,34(3):198-209

We have developed an algorithm for taking into account the neutrino scattering in the approximation of neutrino heat conduction. We show that in the case of incoherent neutrino scattering (e.g., by electrons), the coefficients of the temperature and chemical potential gradients are averaged over the neutrino energy using functions that can be found by numerically solving integral equations. The coherent scattering by free nucleons and atomic nuclei can be described by introducing a transport cross section. We suggest a new method for calculating the neutrino—electron scattering functions that is based on Fermi—Dirac functions of integer indices.  相似文献   

高放废物地质处置阿拉善预选区巴彦诺日公地段目标深度岩体质量预测     

袁广祥  张路青  曾庆利  黄志全  王四巍  王洪建  邓绪彪 《地质与勘探》2019,55(3):840-849

高放废物地质处置阿拉善预选区巴彦诺日公地段位于阿拉善地块东部,主要由二叠纪侵入的花岗岩构成,地壳次稳定。通过踏勘,确定了2个钻孔,布置了若干条物探剖面。以这2个钻孔为中心,在17km×17km范围内进行了工程地质测绘,获得了地表结构面分布特征。地表岩体质量以III级岩体为主,地表以下3m~4m处多为I级和II级岩体。根据钻孔岩芯编录和力学试验数据,对岩芯质量进行评价,岩芯整体质量较好,以Ⅰ级和Ⅱ级岩体为主。对比岩体质量和测井数据,发现岩体质量与岩体的物理参数具有明显的相关性。通过和CSAMT剖面上对应位置的对比,建立了岩体质量与电阻率的关系。结合地表岩体质量、钻孔岩芯质量和物探剖面,对目标深度岩体进行了预测：目标深度（600m深左右）岩体质量以Ⅰ级岩体为主,局部有Ⅱ级岩体和Ⅲ岩体。  相似文献   

朝鲜2017年核爆对中国东北地区形变场的影响     

王阅兵  甘卫军  张锐  游新兆 《大地测量与地球动力学》2020,40(1):11-16

基于19个连续GNSS观测站的多种采样率（10 Hz、1 Hz和30 s）数据,分析2017-09-03朝鲜核爆对中国东北地区地壳形变场的影响。静态位移分析结果显示,距核爆现场最近的GNSS观测站JLCB没有产生明显的同震形变,与基于均匀半无限弹性空间断裂位错模型正演模拟的结果一致;GNSS应变结果显示,此次核爆在东北区域引起主应变的略微调整,但总体调整量在10-8以内,没有引起区域范围内面应变的变化;高频GNSS动态形变分析结果显示,核爆在JLCB站处没有引起明显的波形变化。另外,高频GNSS受到多路径效应的影响,可能会引起cm级的扰动,利用恒星日滤波方法可以抑制多路径的影响,得到精度更高、更可靠的动态形变结果。  相似文献