太阳耀斑

They indicate that the energy of proton from SUN can be accelerate much more than 10 GeV.

目前有一些实验报道在大的耀斑期间观测到具有方向性μ子暴，如果它们和太阳活动相关，则来自太阳的质子能量应该大于几十、几百GeV甚至更高。

The detailed time-match semiempirical models represnting the chromospheric state during the impulsive phase of the 2B flare on Fab. 3 1983 are proposed by making the non-LTE calculstions on hydrogen and ionized calcium. The physical pictures of total evolutionary pattern of the impulsivs phase of the flare are improved either quantitatively or qualitatively in comparison with the former work we did.

利用南京大学太阳塔多波段光谱仪拍摄到的1983年2月3日2B级耀斑脉冲相期间的Hα和CaⅡK线轮廓系列光谱资料，按照我们所发展的构造定态色球耀斑半经验模型的方法，通过联立求解氢和一次电离钙的能级平衡方程和辐射转移方程，建立了能够再生Hα和CaⅡK线观测轮廓的更为完整的1983年2月3日2B级耀斑脉冲相色球半经验模型。

The data such as the Hα-spectrum-spectroheliographic observations, the Hα-chromospheric observations, etc., of a flare loop prominence which occurred on the western solar limb on 1981 April 27 have been obtained at Yunnan Observatory, Academia Sinica.

云南天文台摄取1981年4月27日太阳西边缘的一个耀斑环珥的H_α光谱太阳分光照像(S~2HG)和H_α色球照像等资料。

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。

Based on a qualitative analysis of the data of the type IV radio burst and accompanying phenomena (post flare loops, radio pulsation in the decaying phase,multi-band emissions and mass ejection etc.)associated with the white light flare of 1991 June 6, it isproposed that the WLF and radio burst come from the sameelectron accelerating area in the low corona.

通过1991年6月6日共生太阳白光耀斑的射电运动IV型爆发及其伴随现象(包括耀斑后环、爆发衰减相的射电脉动、多波段射电辐射和太阳物质抛射等)观测资料的分析，定性地探讨了WLF的起源、加热机制和发射地点的问题。

Based on the observations of solar magnetic fields and soalr flares, solar physicist have proposed four model of magnetic field structure by which solar flare can take place.

因此人们根据太阳磁场和耀斑的观测设想了四类产生耀斑的磁场结构模型。

Brace yourself, because in roughly five to six years, your beloved handheld devices won't work for several hours due to solar flare activity (sound familiar?).

因为在大约5到6年后，你们心爱的手持设备在太阳耀斑大爆发的几个钟头之间无法工作

Magnetic field plays a central role in solar activity. Almost all kinds of solar activities, such as sunspot, solar flare and coronal mass ejection, are associated with solar magnetic fields.

磁场在太阳活动中扮演着主要的角色，太阳表面上各种活动现象（如太阳黑子、耀斑爆发和日冕物质抛射等）都和太阳磁场有关。

Magnetic field plays central role in solar activity. Almost all kinds of solar activities, such as sunspot, solar flare and coronal mass ejection, are associated with solar magnetic field.

磁场在太阳活动中扮演者最主要的角色，太阳表面上各种活动现象(如太阳黑子、耀斑爆发和日冕物质抛射等)都和太阳磁场有关。

"I fear we are going to get a repeat of Canada in 1979 when a giant solar flare took out the power grid of the entire eastern seaboard," Mr Bennedick said.

&我怕我们将要在1979年获得加拿大重演当一个巨型太阳耀斑取出了整个东海岸电网&bennedick说。

The split between the two groups can hardly be papered over.

这两个团体间的分歧难以掩饰。

This approach not only encourages a greater number of responses, but minimizes the likelihood of stale groupthink.

这种做法不仅鼓励了更多的反应，而且减少跟风的可能性。