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661.
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663.
C.-C. Wu C.D. Fry M. Dryer S.T. Wu B. Thompson Kan Liou X.S. Feng 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2007,40(12):1827-1834
This study performs simulations of interplanetary coronal mass ejection (ICME) propagation in a realistic three-dimensional (3D) solar wind structure from the Sun to the Earth by using the newly developed hybrid code, HAFv.2+3DMHD. This model combines two simulation codes, Hakamada–Akasofu–Fry code version 2 (HAFv.2) and a fully 3D, time-dependent MHD simulation code. The solar wind structure is simulated out to 0.08 AU (18 Rs) from source surface maps using the HAFv.2 code. The outputs at 0.08 AU are then used to provide inputs for the lower boundary, at that location, of the 3D MHD code to calculate solar wind and its evolution to 1 AU and beyond. A dynamic disturbance, mimicking a particular flare’s energy output, is delivered to this non-uniform structure to model the evolution and interplanetary propagation of ICMEs (including their shocks). We then show the interaction between two ICMEs and the dynamic process during the overtaking of one shock by the other. The results show that both CMEs and heliosphere current sheet/plasma sheet were deformed by interacting with each other. 相似文献
664.
提出了如何在给定的行程速比系数条件下,按最小的传动角最大的要求设计曲柄插杆的一个命题,并对该命题进行了证明。 相似文献
665.
为了深入分析燃油喷嘴对燃气轮机燃烧室性能的影响,针对燃气轮机燃烧室中的直射式气动雾化喷嘴开展了数值模
拟,获得了气流流量、燃油流量和气液比对雾化性能的影响规律,喷嘴的雾化性能参数包括雾化粒径和雾化锥角。结果表明:气液
比和气流流量对该型喷嘴的雾化性能有显著影响,燃油流量对雾化性能的影响较小;气液两相间相对速度是影响该型喷嘴雾化性
能的决定因素,相对速度增大有利于减小雾化粒径,并增大雾化锥角;气流流量和气液比的增大均有利于雾化粒径的减小,燃油流
量的增加将使雾化粒径增大;增大气流流量、气液比和减小燃油流量均可使雾化锥角增大;该型喷嘴的雾化锥角变化范围为
30.12°~41.24°,雾化粒径变化范围为131.46~ 186.52 μm。喷嘴可实现在较小的雾化锥角变化范围内获得较宽的雾化粒径变化,
以此匹配燃气轮机燃烧室不同工作状态,具有较高的实用价值。 相似文献
666.
Y. Suzuki 《Space Science Reviews》1998,85(1-2):91-104
The current status of solar neutrino experiments is reviewed. All the experimental measurements show deficits of solar neutrinos.
Non monotonic suppression indicates that the problem may naturally be explained by neutrino oscillations, but not by modifying
solar models. A new experiment shows very promising results. We hope that a definite answer to the question of whether solar
neutrinos are oscillating will be obtained in the very near future.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
667.
Hui Li Youping Li 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(6):962-968
An M7.6 flare was well observed on October 24, 2003 in active region 10486 by a few instruments and satellites, including GOES, TRACE, SOHO, RHESSI and NoRH. Multi-wavelength study shows that this flare underwent two episodes. During the first episode, only a looptop source of <40 keV was observed in reconstructed RHESSI images, which showed shrinkage with a velocity of 12–14 km s−1 in a period of about 12 min. During the second process, in addition to the looptop source, two footpoint sources were observed in energy channel of as high as ∼200 keV. One of them showed fast propagation along one of the two TRACE 1600 Å flare ribbons and the 195 Å loop footpoints, which could be explained by successive magnetic reconnection. The associated CME showed a mass pickup process with decreasing center-of-mass velocity. The decrease of the CME kinetic energy and the increase of its potential energy lead to an almost constant total energy during the CME propagation. Our results reveal that the flare and its associated CME have comparable energy content, and the flare is of non-thermal property. 相似文献
668.
669.
环氧树脂648和TDE-85的质子辐照损伤效应研究 总被引:3,自引:0,他引:3
通过地面模拟空间环境质子辐照条件(质子能量Ep=150keV,束流密度A=2.0×1012cm-2·s-1,辐照剂量范围Φ=(0~5.0)×1016cm-2;真空度10-6Pa,环境温度120 K),研究了不同辐照剂量下环氧树脂浇注体648和TDE-85的质量损失、弯曲强度和表面相糙度的变化.试验结果表明,随着辐照剂量的增加,质量损失呈现先加速递增后趋于平缓的趋势;648的弯曲强度呈单边下降趋势,TDE-85的弯曲强度呈现先上升后下降的趋势,树脂表面产生了碳化效应,表面粗糙度发生了不同程度的变化. 相似文献
670.