geomagnetic storm的例句大全

Study of Ionospheric Irregularities in the Vicinity of SED Region During a Super Geomagnetic Storm

暴时密度增强区附近电离层不均匀体研究

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Longitudinal asymmetry of the main phase of the geomagnetic storm degree of graphitization

磁暴主相的经度不对称性

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The Impact of Geomagnetic Storm on Electrical Power Systems

地球磁爆活动对电力系统的影响

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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。

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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。

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Morphology analysis of mid and low latitude ionospheric response to geomagnetic storm

磁暴期间中低纬电离层暴形态和物理机制分析

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It is widely accept that power systems are affected by the geomagnetic storm.

磁暴会对电力系统产生影响这种观点已经广泛为人们所接受。

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Effects of the Interplanetary Disturbances on Geomagnetic Storm Development

行星际扰动对地磁暴发展的影响研究

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The Geomagnetic Storm's Prediction by The multivariate Statistical Analysis

用多元统计分析予报地磁暴

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Anisotropy Analyses of Cosmic Ray Before the Geomagnetic Storm on Sep.24,1998

1998年9月24日地磁暴前宇宙线各向异性特性分析

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and while aurorae are normally visible only at high latitudes, they can light up the sky even at lower latitudes during a geomagnetic storm.

虽然极光通常只出现在高纬度地区，但是在磁暴发生时，极光也能点亮稍低纬度地区的天空。

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Moreover, when a shock penetrates an MC at the different depth, the resulting geomagnetic storm is also different.

而且，激波进入磁云的不同深度，引起的地磁扰动也不同。

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The global ionospheric response to the geomagnetic storm event during May 1998

1998年5月磁暴事件期间全球电离层响应形态与机制的研究

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By means of the observation data obtained under the ionogram work mode, three large geomagnetic storm events are observed in April, 2006.

通过系统的频高图工作模式下所获取的电离层特征参数观测数据，在2006年4月份的一个月间，观察到了三次大的磁暴事件。

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In this paper, the stratification events of the ionosphere related to geomagnetic storm in the night-time over Wuchang are studied.

本文研究了武昌上空与磁暴有关的电离层夜间分层事件。

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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。

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An analysis of interplanetary sources of geomagnetic storm during November 7 ― 8, 1998

1998年11月7～8日磁暴的行星际源分析

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Global Ionospheric Response to the Geomagnetic Storm Event of April 6-7, 2000

全球电离层对2000年4月6-7日磁暴事件的响应

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Throuth scaling and processing these ionogram data, the characteristics during one of the three geomagnetic storm events ( from April 13 to 17 of 2006) is studied in detail.

利用记录的频高图数据，通过参数标定和信息提取，对这三次磁暴事件中的一次事件（2006年4月13日至17日间发生）进行了较为详细的电离层暴时特性分析研究。

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Low-Latitude Whistlers during the Strong Geomagnetic Storm

低纬地区磁暴期间的哨声

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