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111.
Coronal mass ejections and post-shock streams driven by them are the most efficient drivers of strong magnetospheric activity,
magnetic storms. For this reason there is considerable interest in trying to make reliable forecasts for the effects of CMEs
as much in advance as possible. To succeed this requires understanding of all aspects related to CMEs, starting from their
emergence on the Sun to their propagation to the vicinity of the Earth and to effects within the magnetosphere. In this article
we discuss some recent results on the geoeffectivity of different types of CME/shock structures. A particularly intriguing
observation is that smoothly rotating magnetic fields within CMEs are most efficient in driving storm activity seen in the
inner magnetosphere due to enhanced ring current, whereas the sheath regions between the shock and the ejecta tend to favour
high-latitude activity. 相似文献
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初步探讨了飞机机翼翼梁接头高强度铝耳片与钢衬套过盈配合在应力腐蚀与干涉连接综合作用下 ,对耳片疲劳寿命的影响及影响程度 ,并提出了结构设计时应遵循的几项原则。 相似文献
115.
Terrestrial technology is now, and increasingly, sensitive to space weather. Most space weather is caused by solar storms
and the resulting changes to the Earth's radiation environment and the magnetosphere. The Sun as the driver of space weather
is under intense observation but remains to be adequately modelled. Recent spacecraft measurements are greatly improving models
of solar activity, the interaction of the solar wind with the magnetosphere, and models of the radiation belts. In-situ data
updates the basic magnetospheric model to provide specific details of high-energy electron flux at satellite orbits. Shock
wave effects at the magnetopause can also be coarsely predicted. However, the specific geomagnetic effects at ground level
depend on the calculation of magnetic and electric fields and further improvements are needed. New work on physical models
is showing promise of raising geomagnetic and ionospheric predictability above the synoptic climatological level.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
116.
Kamide Y. Kihn E.A. Ridley A.J. Cliver E.W. Kadowaki Y. 《Space Science Reviews》2003,107(1-2):307-316
We report the recent progress in our joint program of real-time mapping of ionospheric electric fields and currents and field-aligned
currents through the Geospace Environment Data Analysis System (GEDAS) at the Solar-Terrestrial Environment Laboratory and
similar computer systems in the world. Data from individual ground magnetometers as well as from the solar wind are collected
by these systems and are used as input for the KRM and AMIE magnetogram-inversion algorithms, which calculate the two-dimensional
distribution of the ionospheric parameters. One of the goals of this program is to specify the solar-terrestrial environment
in terms of ionospheric processes, providing the scientific community with more than what geomagnetic activity indices and
statistical models provide.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
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闫海青 《沈阳航空工业学院学报》2000,17(4):46-49
本文对激光全息干涉图的采取以及干涉等值线条纹图的处理进行了研究,并采用进行的细化算法对等值线进行细化,解决了以前算法细化不全和速度慢等问题,使以干涉等值线为基础的光学数据更加安全,可靠。 相似文献
119.
为研究侧向喷流对高超声速拦截弹喷流直接力控制性能的影响,发展了在有限体积离散方法框架下的三维非定常N—S方程,采用LU—SSOR隐式时间推进格式和残值项空间迎风型格式求解技术,对大气层内高超声速拦截弹多个姿态控制喷流发动机同时工作时的干扰流场进行了数值求解。计算给出了自由流与侧喷流、侧喷流与侧喷流之间复杂干扰流场结构图(等压云图、等马赫云图)以及喷流附近的压强分布,其结果与单一侧向喷流流场情况进行了比较和分析。结果显示,喷流前的压强场基本不受后喷流的影响,处于前喷流尾流区后的喷流的干扰效率将受到较大影响。 相似文献
120.