2016-05-24 14:54
substorm翻译
亚暴
音标读音
英式:['sʌbstɔ:m]美式:['sʌbstɔ:m]
基本意思
n.亚暴（地球磁层中的一种扰动）
形近的词
变形
例句
- In this paper, a mechanism of the earth's magnetospheric substorm is discussed.
本文讨论了一种地球磁层的亚暴机制。
- In the paper a model for the three-dimensional substorm current system producing low-latitude Pi2 pulsations has been constructed.
本文试图建立一个产生低纬Pi2脉动的亚暴三维电流体系模型。
- The particles are heated and accelerated in the plasma sheet, and then injected into the near earth space, and produce the ring current and auroral substorm.
等离子体片中的粒子被加热和加速后，注入近地空间，产生环电流和极区亚暴。
- The authors consider that the stratification events may be caused by precipitation of particles and closely related to polar substorm.
作者认为，分层事件似应是由沉降粒子所引起，并与极区亚暴具有密切关系。
- The surface conductivity changes and the regularities of two common thermal control paints have been studied in simulated substorm condition. Several significant results have been obtained.
据此，本文对两种常用的航天器表面涂层在模拟空间亚暴环境下电导性能的变化及其规律作了实验研究。
- Relation between the variation of geomagnetospheric relativistic electron flux and storm/ substorm
磁层相对论电子通量变化与磁暴/亚暴的关系
- THEMIS data revealed that the February substorm was sparked by an explosion along field lines in Earth's magnetic tail at a distance some 10 to 15 times greater than the planet's diameter.
“西弥斯”的数据显示，发生在二月份的磁暴来自一个沿着场力线尾部的爆炸，爆炸的范围约为地球直径的10到15倍。
- Chapter 2 introduces the space environment of geomagnetic substorm and its detrimental surface charging effects.
第二章介绍了空间地磁亚暴环境及其引起的航天器表面充放电效应和危害。
- This paper provides the assessments of multi-energy electron simulation method for GEO substorm charging effect study.
文章着眼于提高地球同步轨道（GEO）空间地磁亚暴带电效应模拟的真实度，对多能量电子模拟空间地磁亚暴带电的方法进行分析评估。
- Mechanism of magnetospheric substorm and the turbulence of solar wind
太阳风湍流和磁层亚暴的一种机制
- The occurrence rate is only 8.9% at the lowest level, while 73.2% of events occurred above active level. Most events are accompanied with substorm in the night.
在最低活动水平，发生率只有8.9%，而73.2%的事件发生在扰动水平以上。
- The Correlation Between Field Aligned Currents and Geomagnetic and Substorm Activity
场向电流与地磁和亚暴活动的相关性
- 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；
- Magnetic reconnection can transfer magnetic energy into plasma thermal and kinetic energy in short time period, and changes the topology of magnetic field, thus it is suggested as related many explosive phenomena, such as solar flare, magnetosphere substorm.
磁场重联可以在短时间年内将磁能转化为等离子体的动能和热能，并改变磁场的拓扑结构，被认为与许多爆发性现象有关，比如太阳耀斑和磁层亚暴等。
- A simulation study of multiple plasmoids in the magnetotail during substorm event(ⅰ)
亚暴事件中磁尾多重等离子体团的数值研究（Ⅰ）
- The Influence of Dawn-Dusk Electric Field on the Triggering of Magnetospheric Substorm
晨昏电场对磁亚暴触发的影响
- 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。
- The Kelvin-Helmholtz instability in boundary layer regions of the plasma sheet during magnetospheric substorm recovery is studied based on two idealized MHD models.
本文根据两个理想的磁流体力学模型研究了磁层亚暴恢复期间等离子体片边界层区的Kelvin-Helmholtz不稳定性。
- The energy released by the plasmoids and associated tailward fast flow was estimated to be roughly 1015J, which is the same order as the energy released to the auroral ionosphere in a substorm.
据估计，通过等离子体团及与之相关的快速尾向流，释放的能量约为1015J，与亚暴期间向极光电离层释放的能量具有相同的量级。
- Three-dimensional current system at high-latitude during substorm
磁层亚暴期间高纬地区三维电流体系
- Said the satellite surface charging environment means the environment of the satellite surface charged. It mainly means the plasma environment when the magnetic substorm occurred.
所谓卫星表面充电环境是指使卫星表面充电的环境，它主要指磁层亚暴时的等离子体环境。
- A near-Earth triggering model for the magnetospheric substorm expansion phase
磁层亚暴膨胀相的近地触发模型
- Since the AE increase of a typical substorm is larger than 200 nT, whether a substorm can be triggered depends mainly on the conditions of the braking regions prior to fast flows.
由于在一个典型亚暴中，AE指数的增加通常大于200nT，高速流是否可以触发亚暴，主要依赖于其停滞区的空间环境条件。
- The mechanism of acceleration of ring current during a substorm of magnetosphere
磁层亚暴时环电流的局部加速机制
- A relation between the auroral X-ray total intensity and the substorm index-AE
X射线极光强度与亚暴指数AE的相关关系
- The relationship between field-aligned current and substorm phase
场向电流随亚暴位相的变化
- 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。
百科解释
网络意思