1)Flare[英][fle?(r)][美][fl?r]耀斑
1.Study of the Response of the Ionosphere Over Sun-Lit Boundary Region to Solar Flare;日照边缘区域电离层对耀斑的响应特点研究
2.Theory for ~3 He-Enrichments in Solar Flares;太阳耀斑中~3He富化的理论(英文)
3.Study of the Flare and Its Velocity Fields Observed on August 17, 1989;1989年8月17日太阳边缘耀斑和速度场研究
英文短句/例句
1.EUV emission of the solar flare太阳耀斑极紫外辐射
2.X-ray emission of solar flare太阳耀斑Ｘ射线辐射
3.The filament near the flare became active long before the start of the flare.(1)在耀斑开始很早以前,耀斑附近的暗条就变得活动起来。
4.east-west asymmetry of solar flare with proton events粒子耀斑的东西不对称性
5.STUDY OF THE WHITE LIGHT FLARE OF SEPTEMBER 10,19741974年9月10日白光耀斑研究
6.The Evolution of the Proton Flare Active Region McMath 111281971年1月质子耀斑活动区的演化
7.H_α Post-Flare Loops on May 16,19811981年5月16日耀斑中的环弧系
8.AN ANALYSIS ON VELOCITY FIELD OF THE POST FLARE LOOP SYSTEM OF AUGUST 17, 19891989年8月17日耀斑后环系速度场分析
9.The Improvements of the Measuring Method of the Flare Data Obtained at Yunnan Observatory云南天文台耀斑数据测量方法的改进
10.The Relation Between Solar Flare and. Longitudinal Current Density on Jan. 14, 19891989年1月14日耀斑和纵向电流的关系
11.THE RELATION BETWEEN MORPHOLOGICAL EVOLUTION OF ACTIVE REGION 6850 AND THE FLARES6850活动区的形态演化与耀斑的关系
12.The Line of sight Velocity Fields of the Flare Loops of 1989 August 171989年8月17日耀斑环的视向速度场
13.An Analysis of A Large Flare, on the Solar Disc of 1984 February 251984年2月25日日面大耀斑光学特性
14.VERY HIGH-ENERGY PARTICLE EMISSION FROM THE SOLAR COSMIC RAY FLARES太阳宇宙线耀斑中的甚高能粒子发射
15.Study on the Condition of γ-Ray Emission in Solar Flare;太阳耀斑产生高能γ射线的过程研究
16.Contribution Function and Three-Dimensional Reconstruction of Hα Chromospheric Flare;贡献函数及Hα色球耀斑的三维重构
17.Correlation between Solar Photospheric Magnetic Properties and Flare Productivity;太阳光球磁场特性与耀斑相关性研究
18.Sunspot Group No. 184 in April 1980 and the Flare on April 7 in 19801980年4月份184号黑子群及4月7日耀斑
相关短句/例句
solar flare耀斑
1.The author of this paper analyzed the relativity between sunspot and solar flare and earthquake,and concluded that the statistical relationship between solar activities and small earthquakes in that area didn t exist,strong earthquakes had puny relativity with solar activities.作者选取云南省及周边地区1965~2006年2级以上地震为样本,使用时间序列分析方法和相关分析方法对地震与太阳黑子、耀斑的相关性进行了研究,得到中小地震为主的样本与太阳活动不相关、大地震与太阳活动存在弱相关性的结论。
2.The data from the International GPS(global positioning system) Service(IGS) are used to investigate the characteristics of the sudden increase of the ionospheric total electron content(Q_(TEC)) response to the solar flare.利用全球定位系统(GPS)台网数据,研究了耀斑爆发期间电离层总电子含量(QTEC)的突然增强(SITEC)现象。
3)flares[英][fl??s][美][fl?rs]耀斑
1.The Low Energy Cutoff of the Nonthermal Electrons of the RHESSI Flares;RHESSI耀斑中非热电子低能截止的研究
2.The study of solar filament activations and eruptions is important not only in understanding formation and stability of filaments but also in understanding violent solar eruptions such as flares and coronal mass ejections.太阳暗条激活与爆发的研究 ,不仅对理解暗条的形成、支撑和稳定性是重要的 ,对理解剧烈的太阳爆发 ,如耀斑和日冕物质抛射 ,也是重要的。
4)X flaresX耀斑
5)glint removal耀斑去除
6)Solar flare太阳耀斑
1.Responses of lightning flashes number to solar flare over Beijing-Tianjin-Hebei;京津冀地区闪电计数对太阳耀斑爆发的响应
2.Monitoring result and analysis of two different solar flare using GPS;利用GPS监测两起太阳耀斑事件的结果分析
3.Monitoring and analysis of the solar flare by GPS data of CCDMN;利用中国地壳运动观测网络的GPS资料对太阳耀斑的监测及分析
延伸阅读
耀斑耀斑solarflares在太阳大气（很可能在色球-日冕过渡层）中非常集中的能量突然释放以及而后物质运动和温度逐渐衰减的过程。倾向认为它是色球-日冕不稳定性的次级效应。耀斑常出现在磁场梯度大、结构复杂及具有高应力和不稳定磁场位形的活动区中。存在这些条件的标志有：出现反常极性的双极场；老活动区中或其附近长出新的磁场；Ha谱斑大且亮；代表磁场中性线的暗条走向曲折及暗条突然膨胀或消失等等。有时在同一个活动区可能发生几次耀斑。一般把增亮面积超过3亿平方千米的称为耀斑，而面积小于3亿平方千米的则叫亚耀斑。与耀斑有关的光学现象有：耀斑前暗条激活、冲浪、喷焰、爆发日珥和环状日珥等。与耀斑共生或由耀斑引起的现象包括太阳紫外线、软X射线、硬X射线、γ射线和射电波段的爆发；各种高能粒子（质子、电子、中子）辐射的突然增强；磁暴、突然电离层扰动、极光、极冠吸收等地球物理效应。
