日冕

Solar Wind Origin in Coronal Funnels: An Introduction of the Article Published in Science, Vol

篇名 太阳风在日冕磁漏斗状结构中的起源－介绍一篇Science，Vol 308，2005上的研究论文

Unfortunately the corona hisses and distorts the music.

不幸的是日冕hisses和歪曲了音乐。

Two similar major coronal mass ejections occurring on October 28 and November 18, 2003 were reported.

研究了分别发生在2003年10月28日和2003年11月18日的两次相似的强烈日冕物质抛射事件。

Flares and mass ejections are no danger for humans or other life on Earth.

耀斑和物质抛射是没有人类或地球上其他生命危险，日冕物质抛射。

It is expected to peak around 2012, bringing lots of sunspots, flares and coronal mass ejections.

下次出现活动高峰期预计在2012年，到时会出现大量的太阳黑子，太阳耀斑以及日冕物质抛射。

Some activity, like mass ejections, are directional. Earth may not be in the path of a particular ejection so all activity does not affect Earth.

有些活动，像是日冕物质喷射是具有方向性的，地球也许并不在其特定的喷射途径中，所以并不是所有的太阳活动都会影响地球。

The study of solar filament activations and eruptions is important not only in understanding formation, supporting and stability of filaments in general, 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。

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。

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。

Life. But the intrinsic way of the Internet by wire confines accessing and using of the network information.

然而，Internet固有的有线连接方式大大限制了人们对网络信息的访问和使用。

I have a strong persuasion that this is true .

我坚信这是正确的。