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- The periodic analysis for the data of cosmic ray flux after meteorological effect inspection shows that solar time semi-diurnal, 0.996 and 1.002 diurnal variations exit in the data of TeV and lOTeV cosmic ray. 对气象效应修正后的宇宙线流强数据进行周期分析，发现TeV和10TeV宇宙线数据中存在半日、0.;996和1
- 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. 宇宙线强度随时间的变化、时间变化的起源和与天体物理因素的联系是宇宙线物理、地球物理和天体物理学科中最复杂的问题之一,具有重要的物理意义。
- Is the Continuum Emission of Solar Flare a Sort of Unusual Events? 耀斑的连续发射是罕见的吗?
- The time jetter of the cosmic ray detecting system is 79.5 ps. 宇宙线测量系统的时间晃动为 79.;5ps
- One possibility is that the blast was like an ultra-powerful solar flare. 一种可能的原因是这种爆炸很像有超级能量的太阳耀斑。
- solar flare effects 太阳耀斑效应
- The sidereal diurnal variation (T=0.997d) for lOTeV cosmic ray has been detected with about signal-noise ratio 5.0, with amplitude 0.125 + 0.079% and phase 0.45(llh) by analyzing the data of cosmic ray flux after meteorological effect corrected. 通过对气象效应修正后的宇宙线流强数据进行周期分析，发现了10TeV宇宙线流强的恒星日(T== 0.;997日)变化，其信噪比为5
- Conversely, when solar activity is less intense, more cosmic rays get through. 一项研究发现，当宇宙射线最弱和最强时，地球上空为云层所覆盖的区域比例分别是65%25和68%25。
- The storm, the most disruptive to hit Earth since1989, was unleashed by the fourth-most powerful solar flare ever seen. 迄今为止第四最强烈的太阳耀斑所释放出来的太阳风暴，是自1989年以来所有袭击地球的太阳风暴中最具有破坏性的。
- Scientists are using cosmic ray detectors to uncover the secrets of the earliest large metropolis of the Americas. 目前，考古学家和核物理学家们正在利用宇宙射线探测器的介子束在太阳金字塔底深处进行勘测，希望能解开这座金字塔的秘密以了解扑朔迷离的狄奥提瓦康古城。
- The most powerful solar flare as observed by satellite instrumentation is recorded. 2003年的今天，由卫星仪器观测到的最强的一次太阳耀斑被记录。
- Ordinary cosmic rays are puny things. 普通的太空射线都是微不足道的东西。
- Sometimes, cosmic rays affect the earth. 宇宙射线有时候也会对地球产生影响。
- It was the most brilliant solar flare ever recorded, bespeaking enormous energies released into the solar atmosphere. 这是有记录以来最亮的一次日焰，代表著极大量的能量被释放到太阳大气中。
- The number of cascade particles changes according to the incident cosmic ray energy, observation height, etc. 到达地面的簇射粒子数目会随不同因素而改变，包括原初宇宙射线的能量、观测高度等。
- An exception to the above pattern occurs during solar flare activity, which takes place on an occasional basis during periods of high solar activity. 例外情况然而亦有,这就是在太阳活跃期偶发的闪焰爆发。
- Using Monte-Carlo method, the propagation of cosmic ray hadrons throughatmosphere is simulated. 用蒙特卡洛 (Monte-Carlo) 方法,模拟了宇宙线强子成分在大气中的传播。
- Solar flares can also doom satellites. 太阳火焰还能使人造卫星毁于一旦。
- Further application of pulsed laser technique to the study of high energy physics and cosmic ray physics are discussed. 最后,就脉冲激光技术在高能物理和宇宙线物理研究中的进一步应用作了讨论。
- How do solar flares reach Earth? 太阳闪焰如何抵达地球?
