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- 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
- THE ORIENTATION OF THE IMF turns southward quite frequently, so magnetospheric substorms are fairly common: on average, they happen a few times every day and last for one to three hours. 因为IMF经常转向南方,所以磁层次磁暴相当常见:平均一天可以发生好几次,每次持续一至三小时。
- Keywords Magnetospheric substorm;expansion phase;Near-Earth magnetotail drift mode instability;Cross-tail current disruption.; 磁层亚暴;亚暴膨胀相;近磁尾漂移不稳定性;越尾电流中断;
- magnetospheric substorm 磁层亚暴
- Periodic magnetospheric substorms during fluctuating interplanetary magnetic field Bz 在上下摇动行星间的磁场Bz期间周期性的磁层亚暴
- Yeh, T., 2000: Magnetospheric configuration with magnetotail current, TAO, 11, 423-438. 黄思杰,1999:磁尾电流对地球磁层结构之效应,硕士论文,国立中央大学。
- "The proposed new name is catchy and could be a worthwhile addition to the magnetospheric taxonomy," she said. 她说:“这个已经提出的名字非常吸引人,而且能为磁层分类学添上有价值的一员。”
- So far, technological hurdles have made it hard for scientists to precisely connect a substorm with its most probable cause. 目前止为,由于技术上的障碍,科学家们很难精确了解造成磁暴的最可能的原因。
- The key problem is if the ions upflow can really trigger the substorm onset? A 3-D resistive MHD simulation is carried o. 我们利用三维MHD方法首次对上行离子流触发的亚暴膨胀相起始过程进行了研究。
- This group is devoted to study the generation mechanisms, temporal evolutions and the relations with solar activities of magnetospheric space storms. 本组主要任务是深入了解磁层空间暴(磁暴,亚暴和粒子暴)的产生机制和时空演化过程,及与太阳活动的关系。
- This leads into a thorough description of the Sun and the solar wind, and, finally, the author addresses magnetospheric physics. 这领导进太阳的彻底的描述和太阳风,和,最后,作者地址磁性层的物理学。
- Scientists call them substorm s, a part of larger storms of energy propel led from the sun at supersonic speeds toward Earth and elsewhere in the solar system. 科学家称它们亚暴,是规模更大的太阳能风暴的一部分,以超音速向地球以及太阳系其它地方推进。
- Burch earned his Ph.D. in space science from Rice University in 1968.His main research interests are auroral processes, magnetic reconnection and magnetospheric imaging. 柏奇1968年在莱斯大学取得太空科学博士学位,主要的研究兴趣是极光、磁力线重连以及磁层摄影。
- Even if they survive interplanetary micrometeoroids and fierce magnetospheric plasma, the subtle force exerted by radiation causes their orbits to spiral inward. 即使行星际的微流星体和猛烈的磁层离子体没把它们消灭,辐射的细微影响也会让小粒子迴旋掉下。
- 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。
- The positions at which the spacecraft first crossed the "bow shock" of the magnetospheric interaction with the solar wind, passed closest approach to the planet, and crossed the outbound bow-shock crossing are indicated. 阵地上飞船首次跨过"弓形激波"的磁层与太阳风的相互作用,通过最亲密的态度来处理这个星球,并穿越外弓形激波两边的表示。
- 3.Geomagnetic storm and substorm; 3.;地磁暴与亚暴;
- magnetospheric coordinate systems 磁层坐标系
- Solar magnetospheric system of coordinates 太阳磁层坐标系
- Active Magnetospheric Particle Tracer Explorer; 主动磁层粒子示踪探测器;