太阳耀斑

词组短语

solar flare

与太阳耀斑相关的网络例句 [注：此内容来源于网络，仅供参考]

Solar radio bursts are usually accompanying with solar flares. The complicated radio spectrum detected in solar radio bursts contained a lot of important information on their source region including physical environment and emission mechanism. Especially, because of their morphologic features of short duration, rapid frequency drift, complicated types and so on, the microwave fine structures could bring out rich important information on the source region such as the complicated configuration of magnetic reconnection, the movement of energetic particle, etc.

太阳射电爆发通常发生在太阳耀斑期间，它携带着爆发源区的物理环境以及辐射机制等诸多重要信息，尤其是微波爆发的精细结构，持续时间短、变化快、结构复杂，可以反映重联过程复杂的磁场结构、高能粒子运动等许多特征。

At the peak of the cycle there are typically more sunspots on the Sun, and hence more solar flares.

在繁忙的周期有更多的太阳黑子通常太阳上，因此，更多的太阳耀斑。

Periods of intense solar flares may disrupt communications on Earth and some other things, but the release of a powerful solar storms has scorched the whole earth is nonsense.

剧烈的太阳耀斑可能会破坏地球上的通讯以及其他一些事物，但释放出强大的太阳风暴烤焦整个地球却是无稽之谈。

Chinese painting method is used to form an art that coincides with human thinking. The picture of the sun includes sun's spot, photosphere, sunglow, showing the activities and passion of the sun.

运用中国画写意之法泼彩、晕染、构成、描绘一幅与人类思维相映合，包孕太阳耀斑、黑子、光球、日冕、日珥等诸多运动表像充满激情的太阳图画。

Moreover, the incidence of solar flares and the flux of solar cosmic rays, ultraviolet radiation and x-radiation all vary directly with the sunspot cycle.

此外，太阳耀斑的入射和太阳宇宙射线的流量，紫外线和x光线都直接随着太阳黑子的周期而变化。

The first part of this paper includes reviews of the scientific investigations on solar flares, prominences and coronal mass ejections and on the steady and transient flows of solar wind in interplanetary space, discussions of the solar and interplanetary origins of the space weather, and descriptions of the history and the latest development of MHD simulation in solar-terrestrial space physics.

本文首先回顾了太阳耀斑、日珥和日冕物质抛射三类太阳活动现象以及太阳风的稳态流动和瞬态流动等行星际空间现象，讨论了空间天气的太阳和行星际起源，介绍了日地物理研究中数值模拟发展的历史及最新进展。

This gives you the option of including the sun in the panoramic sky image or placing a light in the approx position of the sun and fine tuning flare controls for your light in your 3d application to mimic the sun size and flare options you require for your scene.

这使您的选择，包括太阳在天空全景图像或放置一个轻的约的立场，太阳耀斑和微调控制的光在您的3D应用模仿太阳的大小和照明选择您需要为您现场。

Using 59 good quality observation data from IGS tracking station, this paper analyses the result of TEC that is caused by X5. 7 solar flare on Jul. 14 2000 and X14. 4 solar flare on Apr.

利用59个数据质量良好的IGS跟踪站的观测数据，对2000年7月14日爆发的X5.7级的太阳耀斑和2001年4月15日爆发的X14.4级的太阳耀斑所引起的TEC的变化情况进行了计算和分析。

A few years ago, some preliminary observations linked a solar flare to a large magnetic disturbance that seemed to have spiraled up from below the sun's surface.

几年前，一些初步观测将太阳耀斑跟磁扰现象联系在一起，磁扰好象从太阳表面以下产生，呈螺旋状上升。

Solar flare is one of violent solar activities. It is confirmed that flux of solar cosmic ray less than 10 GeV rises in neutron monitor.

太阳耀斑是太阳活动之一，已经确切地观测到太阳耀斑期间，中子监测器上观测到能量高达几个GeV太阳宇宙线的增强。

与太阳耀斑相关的网络解释 [注：此内容来源于网络，仅供参考]

solar facula：太阳光斑

Solar Energy Meeting 太阳能会议 | solar facula 太阳光斑 | solar flare 太阳耀斑

flares：耀斑

另一方面,Lockwood教授担忧的是,太阳活动相对平静时,其内部抑制的张力可能突然释放,即会突然产生猛烈的太阳爆发现象,如耀斑(flares)和日冕物质抛射(CME).

Solar flares：太阳耀斑

加州柏克莱大学Themis卫星组专案科学家马里特.奥列罗塞特(Marit Oieroset)表示:"裂缝的扩大速度非常快. "但有些类似的裂缝只是暂时的,2007年发现这个裂缝只裂开大约一个小时而已. 而太阳耀斑(Solar flares)对在轨道活动的太空员可能会构成潜在威胁,通常不会威胁到地面上人类的安全.

sun glint：太阳反辉区(卫星云图上的),太阳耀斑区(卫星云图上的)

sun elevation太阳仰角,太阳高度 | sun glint太阳反辉区(卫星云图上的),太阳耀斑区(卫星云图上的) | sun rise日出

solar granulation：太阳米粒

Solar flares 太阳耀斑 | Solar granulation 太阳米粒 | Solar neutrinos 太阳中微子

solar flocculi：太阳谱斑

solar flare proton event ==> 太阳耀斑粒子事件 | solar flocculi ==> 太阳谱斑 | solar flocculus ==> 太阳谱斑

e.g. Sunspots also have an effect on the earth's magnetic field：太阳耀斑对于地球磁场也有作用

The medicine had no side effects on you.这... | e.g. Sunspots also have an effect on the earth's magnetic field.太阳耀斑对于地球磁场也有作用. | e.g. These agreements have affected both the buyers and t...

solar flare：太阳耀斑

太 阳耀斑(Solar flare)是一种最剧烈的太阳活动. 太阳表面突然出现亮斑闪耀,其寿命仅在几分钟到几十分钟之间,亮度上升迅速,减弱较慢. 一旦出现太阳耀斑,对於太阳 表面来说就是一次惊天动地的大爆发. 耀斑释放的能量相当於10万至100万次强火山爆发的总能量,

impulsive solar flare：脉冲太阳耀斑

immersed echelle 浸渍阶梯光栅 | impulsive solar flare 脉冲太阳耀斑 | infralateral arc 外侧晕弧

solar flare event：太阳耀斑效应

solar energy 太阳能 | solar flare event 太阳耀斑效应 | solar flare 太阳耀斑