为了找到这些问题的答案，该科研组整理了自皮埃尔奥杰宇宙线观测站三年前工作时收集的到的所有资料。
To find answers to these questions, the team trawled through the data that have accumulated since the Pierre Auger observatory began operating three years ago.
他是该项目的主要调查员。因为宇宙线是带电的，它们回溯发射源的轨迹会被银河的磁场破坏，所以宇宙射线图像上任何一个热点都需要一个解释。
Because cosmic rays are charged, their inbound trajectory should be jumbled by the Milky Way's magnetic field, so any hot spot on the cosmic ray map demands an explanation.
点源的寻找是宇宙线研究中的一个热门课题。
The search for gamma ray point sources is a popular topic in the study of cosmic rays.
间歇和分形现象是由在宇宙线实验和高能碰撞中末态粒子相空间中的局域大起伏而引起人们关注的。
The local large fluctuation observed in the final phase space of cosmic rays experiment and high energy collisions cause intermittency and fractal to be the focus.
我们简要讨论了对该能谱的可能解释，包括传统的宇宙线扩散模型以及潜在的邻近额外成分。
Interpretations in terms of a conventional diffusive model as well as a potential local extra component are briefly discussed.
簇射芯位重建是基于地面的宇宙线观测实验的关键工作之一。
The reconstruction of shower core is one of the key works of cosmic ray experiment based on terrene.
这种辐射可能成为宇宙线的一个源。
利用最近的实验结果，计算了宇宙线与星际物质碰撞产生的反质子流强。
Using recent experimental results, we calculate the antiproton flux which is produced by the collisions of cosmic rays with the interstellar matter.
原子核理论研究恒星的结构和演化﹐元素的起源和核合成﹐以及宇宙线问题。
The theoretical study of nuclear structure and the origin and evolution of stars elements of nuclear and cosmic ray problem.
所以，VLF波的传播效应可能成为间接探测宇宙线强度变化的有用工具。
The propagation effect of VLF wave could become a useful tool of detecting the intensity variation of cosmic rays.
太阳宇宙线在行星际空间的传播，包括行星际不规则磁场中的扩散和太阳风对流这两种物理过程。
Physical processes of the propagation of the solar cosmic rays in the interplanetary space include the diffusion in interplanetary disordered magnetic fields and the convection in solar winds.
本文描述了在美国SLAC的PEP-4实验中使用的大型外圆柱漂移室的作用、结构、宇宙线测试方法及其结果。
The function, the structure and the cosmic ray test of the outer drift chamber for PEP-4 Experiment at SLAC are described.
本文描述一个利用云室研究高能宇宙线粒子与石蜡的核作用中次级粒子角分布的实验。
A cloud chamber experiment is described, in which the angular distribution of secondary particles produced in nuclear interaction by high energy cosmic ray particles with paraffin has been studied.
基于宇宙线实验积累数据的分析，求得非弹性K对能量的依赖为0。
Based on an analysis of the accumulated data of the cosmic ray experiments, find that inelasticity K decrease with energy as 0.
提出一种单幅光谱CCD图像宇宙线剔除方法。
A method was proposed to find and remove cosmic-rays from single spectroscopic CCD images.
宇宙线兴盖氏管已过连接成为一种新的高度计用来告诉飞行员他们的高度是多少。
Cosmic rays and Geigertubes have been combined in a new altimeter to tell the pilots what their altitudes are.
采用大含量氟利昂气体，用宇宙线测量该探测器的探测效率，输出电荷，时间分辨。
The efficiency, output charge and time resolution were measured by cosmic muons when the detector was operated with F134a rich mixture in avalanche mode.
本文描述—个宇宙线广延大气簇射观测阵列控制系统。
This paper describes the control system of Zhengziou Cosmic ray Air Shower Array.
应用电子计算机计算了太阳宇宙线在均匀并无限的行星际介质中传播的各向异性扩散对流方程的量纲分析解。
Computer calculations have been made on the dimensional solution to the anisotropic diffusion convection equation for solar cosmic rays propagating in an uniform and unbounded interplanetary medium.
宇宙线强度随时间的变化，是宇宙线物理、太阳地球物理和天体物理等交叉学科中的重要问题之一。
The time variation of the cosmic ray flux is one of crucial problems in the field of cosmic ray physics, solar geophysics and astrophysics, etc.
宇宙线受太阳调制和其它因素影响，流强存在着变化，这种变化可能会引起地球气候的某些变化。
The cosmic ray flux has some changes due to the solar modulation and other factors, and maybe induce some variability of the Earth's climate.
本论文的全部实验工作都是基于宇宙线测试完成的。
All the experiments I report were made using the cosmic ray test system.
宇宙线的恒星日变化紧密联系于宇宙线的起源、其传播途径的性质，以及宇宙线的加速机制等宇宙线物理中最基本的重大问题。
The sidereal diurnal variation of cosmic ray ties up with the most basic and important problem in cosmic ray physics such as the origin, propagation and the acceleration mechanisms of cosmic ray.
给出了不同能区原初宇宙线各种成分产生族事例的效率及其与原初能量的关系。
The production efficiency of family events for different primary particles and its relationship with primary energies are given.
引发单粒子翻转的空间高能带电粒子环境包括银河宇宙线，太阳宇宙线和地球辐射带中的高能质子及重离子。
The space energetic particle environment inducing SEU includes galactic cosmic ray, solar cosmic ray and high-energy trapped protons and heavy ions.
由于甚高能宇宙线的低流强，一直以来甚高能以上能量宇宙线时间变化的研究缺乏统计意义。
However, it lacked significance of statistical to study the time variation of the cosmic ray with even high energy before, because the cosmic ray flux with even high energy is very low.
大气契伦柯夫脉冲波形和光强探测器用于研究跨越宇宙线能谱膝区的核作用特征。
The atmospheric Cerenkov pulse shape and the light intensity detectors were used to investigate the characteristic of the nuclear interactions span knee region of cosmic ray energy spectrum.
简要描述了北京谱仪(BES)主漂移室的结构和宇宙线实验安排，给出利用宇宙线测试主漂移室性能的主要结果。
The structure of the BES main drift chamber and arrangement of cosmic ray tests have been described briefly. The main test results of the chamber performance have been given.
该实验装置与所开发的触发逻辑电子学及在线数据获取系统可以应用于教学和其他相关的宇宙线物理研究。
The apparatus, along with the trigger logic electronics and the online data acquisition, can also be used in teaching experiment and other cosmic-ray related study.
该实验装置与所开发的触发逻辑电子学及在线数据获取系统可以应用于教学和其他相关的宇宙线物理研究。
The apparatus, along with the trigger logic electronics and the online data acquisition, can also be used in teaching experiment and other cosmic-ray related study.
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