solar storm的例句大全

We are now at what should be the peak of what scientists call "Cycle 24"-which is why last week's solar storm resulted in sightings of the aurora borealis further south than usual.

我们现在正处于科学家所谓的第24个太阳活动周期的高峰期，这就是为什么上周的太阳风暴导致比平常更偏南的地方出现北极光。

The amount of radiation regularly reaching Earth from the sun3.45 billion years ago would be comparable to what rains down on the planet during the most powerful solar storms today, Tarduno says.

5亿年前从太阳定期抵达地球的辐射量，将可与现在最大的太阳风暴（solar storm）发生时降落在地球上的太阳雨相比较，塔都诺说。

Research on the relationships between atmospheric electric field anomalies before an earthquake and solar activity and magnetic storm

太阳活动，磁暴与震前大气电场异常关系研究

The solar wind-magnetosphere-ionosphere coupling during magnetic storm

磁暴期间太阳风-磁层-电离层间的耦合过程

It fell silent shortly after a raging dust storm blocked sunlight from reaching its solar panels.

登陆器在一场猛烈的尘暴遮住太阳能电池板的阳光之后不久,就陷入沉寂.

The Phenomenon of Solar Type ⅰ Noise Storm in the Short Decimetric Radio Continuum Emission

太阳短分米波连续辐射中的Ⅰ型噪爆噪声的危害与控制

Low solar wind density and the strong substorm are the two key parameters leading to the 2 MeV electron flux at geostationary orbit reach very high level during the geomagnetic storm recovery phase.

在磁暴恢复相期间，低的太阳风密度和强的亚暴是导致地球同步轨道能量大于2MeV电子通量的达到极高值的两个关键参数。

Reduced risk of solar flares: In 1859, a massive solar flare and geomagnetic storm hit the Earth.

耀斑威胁减小：1859年，一场来自太阳的巨大的耀斑产生的超级磁暴袭击了地球。

The solar flares in February 1986 caused remarkable geomagnetic storm and ionospheric storm.

1986年2月的太阳耀斑爆发导致了强烈的磁暴和电离层暴。

When the AOD value is greater than 1 with high solar zenith angle(> 60 °), the relative error can reach-40%. Satellite observations are an effective way to provide a regional coverage of aerosol optical depth and monitor the occurrence and evolution of dust storm.

当光学厚度大于1并且太阳天顶角较大时（60°），误差能达到-40%。卫星观测是提供全球气溶胶光学厚度分布以及监测沙尘发生的有效途径。

Most extreme high level of electron flux at geostationary orbit occurred during the geomagnetic storm recovery phase with the solar wind proton density lower than 4 cm-3 and strong substorm activity.

绝大多数高通量事件都是出现在磁暴恢复相期间，且太阳风质子密度低于4个/cm3并伴有亚暴时才会发生。

The second is to investigate the trigger mechanisms of magnetic storm, magnetospheric substorm, and magnetospheric particle storm, as well as the responses of magnetospheric space storm to the solar activities and interplanetary disturbance.

研究磁层亚暴、磁暴和磁层粒子暴的触发机制及磁层空间暴对太阳活动和行星际扰动的响应过程；