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flare physics

基本解释耀斑物理

网络释义

1)flare physics,耀斑物理2)solar flare,耀斑3)flares,耀斑4)Flare,耀斑5)coronal mass ejection (CME)/flare,日冕物质抛射(CME)/耀斑6)X flares,X耀斑

用法和例句

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。

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。

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

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。

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

Theory for ~3 He-Enrichments in Solar Flares;

太阳耀斑中~3He富化的理论(英文)

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

EUV emission of the solar flare

太阳耀斑极紫外辐射

X-ray emission of solar flare

太阳耀斑X射线辐射

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。

east-west asymmetry of solar flare with proton events

粒子耀斑的东西不对称性

STUDY OF THE WHITE LIGHT FLARE OF SEPTEMBER 10,1974

1974年9月10日白光耀斑研究

The Evolution of the Proton Flare Active Region McMath 11128

1971年1月质子耀斑活动区的演化

H_α Post-Flare Loops on May 16,1981

1981年5月16日耀斑中的环弧系

AN ANALYSIS ON VELOCITY FIELD OF THE POST FLARE LOOP SYSTEM OF AUGUST 17, 1989

1989年8月17日耀斑后环系速度场分析

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

The Relation Between Solar Flare and. Longitudinal Current Density on Jan. 14, 1989

1989年1月14日耀斑和纵向电流的关系

THE RELATION BETWEEN MORPHOLOGICAL EVOLUTION OF ACTIVE REGION 6850 AND THE FLARES

6850活动区的形态演化与耀斑的关系

The Line of sight Velocity Fields of the Flare Loops of 1989 August 17

1989年8月17日耀斑环的视向速度场

An Analysis of A Large Flare, on the Solar Disc of 1984 February 25

1984年2月25日日面大耀斑光学特性

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

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

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

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

Sunspot Group No. 184 in April 1980 and the Flare on April 7 in 1980

1980年4月份184号黑子群及4月7日耀斑

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