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coronal相关的网络例句

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Coronal mass ejections, known as the most spectacular form of solar magnetic activity, are of great scientific significance in the fields of solar physics.

日冕物质抛射,作为太阳大气中频繁发生的极为壮观的活动现象,越来越受到太阳物理学家的关注。

Radiation with different wavelength is emitted because of reciprocity of coronal mass ejections with corona and interplanetary medium.

分析结果表明,其射电辐射机制主要是轫致辐射、微量的回旋辐射和更加微弱的复合辐射。此外,分析讨论了1999年2月至1999年8月期间与CME共生的太阳微波爆发。

One telescope aboard SOHO can provide three or four days' warning of major solar events by spotting coronal mass ejections.

通过观测日冕物质的喷发,SOHO上的一台望远镜能提前三到四天预报太阳的重大活动。

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。

Although scientists have long sought to figure out what drives both flares and the coronal mass ejections that accompany many of them, only in the past decade or so have observations been good enough to reveal their intricacies and to elucidate the physical mechanism behind them, thanks to new technologies introduced during the 1990s.

虽然科学家早就想要搞清楚,究竟是什麽驱动了日焰以及经常随之而生的日冕团块喷射,但直到最近10年左右的观测结果,才精良至足以揭露它们错综复杂的样貌,并阐明背后的物理机制,这得归功于1990年代才引入的新技术。

The combined perspective of STEREO will help astronomers better understand the mechanisms for the creation and evolution of prominences, coronal mass ejections, and flares.

STEREO卫星的组合视角能够帮助天文学家更好地理解日珥,日冕物质喷发以及耀斑的形成与演变的机制。

On small time scales of a few seconds to several hours,spectacular explosive events occur in the solar atmosphere,such as solar flares,prominence eruptions and coronal mass ejections.

在较小时间尺度上,从几秒到几小时,有时太阳大气中会发生一些壮观的爆发事件,如耀斑、日珥爆发、日冕物质抛射等。

Such special arrangements are probably capable of bringing about a flare, but these mechanisms cannot account for all the observations, especially the tendency for coronal mass ejections to accompany large flares.

此类特殊的安排或许可以产生日焰,但这些机制不能够解释所有的观测现象,特别是日冕团块喷射为何常伴随大型日焰发生。

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。

By analyzing the data from the ACE spacecraft, we describe the characteristics of the magnetic fields and plasma within this MultiMC at 1 AU. We also identify its solar sources, namely coronal mass ejections.

通过分析ACE飞船的观测数据,描述了这个多重磁云在1AU处的磁场和等离子体特征。

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每逢看到沃林顿那刚毅的脸,那乌黑、忧郁的眼睛,她便会相信,他一定作过不幸的爱情的受害者。

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