HADAR实验对活动星系核伽马射线辐射观测的预期研究

HADAR (High Altitude Detection of Astronomical Radiation)是一个基于大气切伦科夫成像技术的地面望远镜阵列,其采用大口径折射式水透镜系统来收集大气切伦科夫光,以实现对10 GeV—10 TeV能量段的伽马射线和宇宙线的探测.HADAR具有低阈能和大视场的优势,因此可以对天区进行连续扫描和观测,在观测活动星系核(Active Galactic Nuclei,AGN)等银河系外伽马射线源方面具有明显优势.本文研究了HADAR实验对AGN的探测能力.基于费米望远镜(Fermi Large Area Telescope,Fermi-LAT)的AGN源能谱信息,将观测能量外推至甚高能能段,同时加入河外背景光的吸收效应,以计算HADAR对AGN源观测的统计显著性.研究结果显示,HADAR运行一年时间,预计将有31个Fermi-LAT AGN源以高于5倍显著性被观测到,其中大部分为蝎虎状天体类型.     

最长弦与最短弦问题

考查经过圆内一点的最长弦与最短弦,尤其最短弦具有的性质是高中数学中的一类重要问题,在近年来的高考及各类数学考试中该类问题频繁出现．试总结如下：     

Cosmic ray electron spectrum due to the dispersion of injection spectrum

The cosmic-ray total electron spectrum(electrons plus positrons) has been measured precisely up to Te V energies,with more interesting features found.Exhaustive analyses of the electron spectrum strongly support a spectral hardening above 100 GeV,rather than a featureless single power-law,which is confirmed by the most recent observations.Meanwhile,the measurements of the DAMPE satellite have verified the presence of a knee-like structure around 1 TeV in the electron spectrum,resembling the cosmic-ray knee.In this paper,we establish a physical model in which the observed electron spectrum is composed of a superposition of CR sources with various spectral indices and high-energy cutoffs.The dispersion of the power index is assumed to be Gaussian,while the cutoff energy Ec follows a power-law distribution.These simple ideas can account naturally for both the hundred-GeV excess and the TeV spectral break.     

羊八井50m~2RPC地毯性能研究YBJ-ARGO合作组(英文)

利用羊八井５０ｍ２ＲＰＣ地毯（ＹＢＪ－ＡＲＧＯ实验原型）的测试数据对其性能进行了分析研究,包括原初粒子方位角分布、天顶角分布、地毯的角分辨、探测时间系统误差对方位角分布的正弦调制、探测时间系统误差的离线修正、几何不对称的小型地毯探测器上原初粒子到达方向重建误差造成的方位角分布的不均匀性等．     

羊八井50m2RPC实验及初步测试结果

介绍了羊八井50m²电阻板室(RPC)地毯实验的结构、安装和对其性能的初步测试.测试的结果表明RPC完全能够很好地在海拔4300m,气压594mbar的羊八井宇宙线观测站正常地运行.     

Lateral distribution of EAS muons measured for the primary cosmic ray energy around 100 TeV

The muonic component of the extensive air showers (EAS) is of great importance for the astroparticle physics. It carries the information about the properties of primary cosmic ray (CR) particles, such as their mass, and electromagnetic and hadronic nature. It provides a sensitive test for the hadronic interaction models, which are inevitable for describing the cascade shower development of cosmic rays in EAS experiments. The YangBaJing Hybrid Array (YBJ-HA) experiment has been in operation since the end of 2016. Surface detectors are used for the measurements of primary energy, angular direction and core position of a shower event, while underground muon detectors are used for measuring the density of muons at various locations. Using the data obtained by the YBJ-HA experiment,this work reports the first measurement of the lateral muon distribution for the primary cosmic ray energy in the 100TeV region. The punch-through effect is evaluated via MC simulation.     

逻辑电路设计中逻辑函数的图形化简法探析

在数字电路中逻辑函数的化简方法一般有公式化简法和图形化简法,其中图形化简法简单、直观,有一定步骤可以遵循,但在教学过程中发现,学生用卡诺图化简逻辑函数时,按教科书中归纳的几个步骤生搬硬套,对最基本的概念和性质缺乏理解,常常出现不少的问题.文章通过案例分析,对逻辑函数的图形化简法进行了深入的分析,并归纳出图形化简法的一般规律.     

最长弦与最短弦问题

考查经过圆内一点的最长弦与最短弦,尤其最短弦具有的性质是高中数学中的一类重要问题,在近年来的高考及各类数学考试中该类问题频繁出现.试总结如下:这里先给出一个常用结论:性质1设圆O的半径为R,M为圆内不同于圆心O的一定点,设OM=m(0相似文献   

溴化钠在正丙醇-水混合溶剂中溶解热和溶剂化热

用高精度等温外壳式量热计测量了２９８．１５Ｋ下ＮａＢｒ在不同组成正丙醇水混合溶剂中溶解热。根据测量结果及以前作者对ＮｄＣｌ３，ＢａＣｌ２，ＮａＣｌ，ＮａＩ，ＮａＦ／ｍ－Ｃ３Ｈ７ＯＨ－Ｈ２Ｏ体系溶解热的研究结果，计算了２９８．１５Ｋ下，正丙醇水混合溶剂中，上述盐的标准溶解热和ＮａＦ，ＮａＣｌ，ＮａＢｒ的ＮａＩ的溶剂化热，讨论了电解质溶解热和溶剂化热与离子特性、混合溶剂的组成和结构的关系。