- 更多网络例句与高能粒子相关的网络例句 [注：此内容来源于网络，仅供参考]
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During the maximum of the 23rd solar cycle, the high energy particle radiation in the South Atlantic Anomy of 860 km altitude had been detected for more than three years by the space particle composition detector.
在第23周太阳活动峰年期间，空间粒子成分探测器对860km高度的南大西洋负磁异常区高能粒子辐射进行了长达3年的连续探测。
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These included an image analysis system to assess the facial mobility of people who are suffering from paralysing diseases or have had surgery on the face; a "text mining" tool to extract chemical information from the world's scientific literature; an educational venture, called Big Bang in a Box, to sell images of high-energy particle collisions at Cern's new atom smasher; and a lightweight material stronger than steel, for use in body armour and the aerospace industry.
其中包括：一套图像分析系统，用于评估罹患了麻痹性疾病者或面部曾动过外科手术者的面部灵活性；"文本采掘"工具，用于提取全球科学文献中的化学信息；创建一家名为"盒中的大爆炸"的教育企业，出售欧洲粒子物理实验室新粒子加速器中高能粒子碰撞的图像；以及一种轻质材料，强度高于钢，应用于防弹衣及航空航天工业。
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We had also performed numerical simulations to study energetic particle injection at L=3.5 to discuss the effect of different pulse parameters on particle injection.
我们也完成在 L=3.5 的电子流量模拟，讨论不同的脉冲参数对於粒子传输的影响和电磁脉冲传输粒子至该处的可能性，以了解是否此电磁脉冲模型可应用於了解磁暴时，在 L=3.5 处高能粒子流量增加的可能性。
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Based on Voyager 1's magnetic field and energetic particle observations, and our knowledge of solar wind shocks, it is inferred that the bulk velocity of the solar wind must have also dropped suddenly when Voyager 1 crossed the TS.
在旅行者一号关于磁场强度和高能粒子的探测数据的基础上，我们原先关于太阳风的知识受到了极大挑战，由它推断，大部分太阳风粒子的速度在旅行者一号穿过终端激波时肯定也急剧降低。
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The energetic light from these stars continually ionizes nebula gas, while their energetic particle wind blows bubbles and defines intricate filaments.
来自这些恒星的高能光不断离子化星云气体，而它们的高能粒子风同时不断地吹向泡泡，产生了错综复杂的细丝景象。
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The first set of data collected by the energetic particle detectors on board of the ZY-1, a China Brasilia coordinated earth resource satellite,were introduced briefly in this paper.ZY-1 is a polar orbiting satellite at an altitude of 780?
对搭载于我国第一颗地球资源卫星上的"星内高能粒子探测器"首批资料进行初步分析表明，在卫星780km轨道高度上所纪录到的所有高能粒子通量事件都只出现在3个地理区域，即两半球的高纬极光带和南大西洋地磁异常区。
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Energetic Particle and Plasma Spectrometer: Measurements of the acceleration of charged particles at the Venus bow shock, where the solar wind slams in to the atmosphere
高能粒子及离子光谱仪：测量金星弓形激波，也就是太阳风轰击大气的地方，处带电粒子的加速度
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The influences of the shock thickness and Alfven waves on the particle acceleration by diffusive shock waves are numerically studied through solving one-dimensional diffusive equation including the second-order Fermi effect. It is shown that the spectral index of the energetic particles strongly depends on the shock thickness. For example, the spectral index increases from 2.1 to 3.7 in the low energy range of 3-10 MeV and from 2.5 to 5.0 in the high energy range of 20-60 MeV as the thickness increases. The spectral index decreases from 4.3 to 3.1 as the particle injection energy increases. The spectral index decreases from 4.0 to 1.8 at the quasi-steady stage with the enhancement of the compression ratio from 2 to 4. The results indicate that under the influence of Alfven waves, the energetic particle spectrum at lower energy becomes flat and the spectral index decreases from 2.5 to 0.6 in the low energy range of 3-10 MeV and from 11.6 to 5.0 in the high energy range of 20-60 MeV. At the same time, the rollover energy reaches 19.6 MeV. The spectral index decreases from 5.8 to 2.9 as the energy density of Alfven waves increase. All these results are basically consistent with the theoretical models, as well as the observations of typical energetic particle events.
通过数值求解包含二阶费米加速的一维扩散方程，探讨在准平行激波条件下激波厚度和级联阿尔芬波对粒子加速的影响，研究粒子分布函数的演化与激波厚度和阿尔芬波强度的内禀关系，计算结果表明：(1)考虑激波厚度时，谱指数明显依赖于激波厚度，随着厚度从0.32增大到2.56，低能端(3-10MeV)谱指数逐渐从2.1增加到3.7，高能端(20-60MeV)谱指数从2.4增大到5.0，能谱逐渐变软；当初始注入粒子动量增大1.3倍，质子能谱指数从4.3减小到3.1，且与零厚度激波加速的谱指数差值缩小；厚度不变时，随着压缩比从2增加到4，准稳态分布时低能端(3-10MeV)粒子能谱指数逐渐从4.0减小到1.8谱变硬；(2)在级联阿尔芬波的影响下，随着时间的增大，粒子在低能处(3-10MeV)的谱指数从2.5减小到0.6高能端(20-60MeV)谱指数从11.6减小到5.0，能谱变硬，拐点能量值从7.5MeV增大到为19.6MeV；随着波的能量密度增大，谱指数从5.8减小到2.9，这表明阿尔芬波强度越大，加速效率越高，通过与激波厚度解析结果和高能粒子事件的观测能谱比较发现两者是一致的，说明数值模拟结果是可靠的。
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Compared to commonγ-ray (x-ray mainly) flash perspectivity techniques, the technique of direct particle detection by CCD has not been widely used by researchers in other fields except several advanced research institutions abroad who use CCD arrays to constitute vertex detectors to record traces of space flight behavior of energetic particles.
相对于目前常用的γ射线透视成像技术而言，除了国外少数先进研究机构采用阵列CCD组建顶点探测器来记录高能粒子的空间飞行径迹以外，利用CCD直接进行粒子探测的技术尚未被其它领域的研究人员所广泛采用。
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The results show that photocatalyst TiO2 improves the removal rate of toluene in not only the nitrogen plasma field (NTP-P-O2/N2) eradiating ultraviolet light but also the argon plasma field eradiating visible light. This supports the idea that both the UV light and the high-energy electron in the plasma field can activate TiO2. Furthermore, the toluene removal rate in NTP-P-Ar system is 5% higher than that in NTP-P-O2/N2 system, confirming that high-energy electron has greater effect on the degradation performance of toluene, as compared with UV light.
结果表明：在发射紫外光的氮等离子体场(NTP-P-O2/N2)中和发射可见光的氩等离子体场中，TiO2：均能提高体系的甲苯去除率，说明等离子体场中产生的紫外光和高能电子均能激活光催化剂TiO2；NTP-P-Ar体系中的甲苯去除率较NTP-P-O2/N2：体系中的约提高5%，说明等离子体场中高能粒子对甲苯降解性能的影响要强于紫外光的影响。
- 更多网络解释与高能粒子相关的网络解释 [注：此内容来源于网络，仅供参考]
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beam：光束
如上所述,"光束(Beam)武器"应理解为高能粒子武器,而与其他一些科幻作品,以及一些电视台所翻译的"激光(Laser)"是两回事.
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energetic particle：高能粒子
这种理论认为,由高能宇宙线产生的高能粒子(energetic particle)大规模簇射,可能触发闪电的大规模能量释放,而这些高能宇宙线则源于一些爆炸的恒星. 要让古列维奇的理论成功运作,必须有大量带电粒子同时通过雷暴,而宇宙线单独产生的大气簇射并不能产生足量的高能粒子.
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energetic particle instrument：高能粒子仪器
enemator 灌肠器 | energetic particle instrument 高能粒子仪器 | Energetine 爱那健丁生血固精片
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energetic particle event：高能粒子事件
energetic particle burst 高能粒子爆 | energetic particle event 高能粒子事件 | energetic particle instrument 高能粒子仪器
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energetic particle burst：高能粒子爆
energetic particle 高能粒子 | energetic particle burst 高能粒子爆 | energetic particle event 高能粒子事件
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particle, energetic：高能粒子
發射粒子 particle, emerging | 高能粒子 particle, energetic | 進入粒子 particle, entering
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energetic solar particle：高能太阳粒子
end-user 最终用户; 最终消费者 | energetic solar particle 高能太阳粒子 | energetic solar proton 高能太阳质子
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high-energy particle：高能粒子
high-energy ignition system 高能点火系 | high-energy particle 高能粒子 | high-energy solar proton 高能太阳质子
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high-energy particle：高能量粒子
high energy nuclear magnetic resonance detector 高能核磁共振仪 | high energy particle 高能量粒子 | high energy particle radiography 高能粒子摄影
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streamer chamber：流光室
流光室(streamer chamber)是在火花室基础上发展起来的高能粒子径迹探测器. 1963年由苏联人G.E.奇科瓦尼(G.E.Chikovani)等人发明. 流光室一般由3个电极将一密闭室隔开成两个间隔,中间电极接高电势,两边电极接地,室内充以氖或氦. 带电粒子进入流光室,