排序方式: 共有85条查询结果,搜索用时 46 毫秒
61.
对少烟丁羟复合推进剂在高压下的燃烧性能,能量特性和微波衰减特性进行了实验研究。研究得出:少烟丁羟复合推进剂在17-18MPa以上压强时存在燃速变现象,但不会引起发动机工作压强失控,而且通过调整弹道良剂可以降低推进剂高压压强指数,少烟丁羟复合推进剂高压少平面实际比冲可以突破2452N.s/kg;该推进剂的微波衰减强度只相当于普通双基推进剂的水平,比(有烟)丁羟复合推进剂和改性双基推进剂低得多。 相似文献
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CME是非重现性地磁暴的诱因,通过对太阳耀斑爆发活动的特征与可能引起地磁活动的CME进行统计分析,发现太阳耀斑的强度、位置、持续时间以及耀斑所伴随的太阳质子事件和行星际高能质子通量的增长与CME的特征及可能产生的地磁扰动有着密切的关系.在对数据分析的基础上,建立了基于人工神经网络的预报模式,对太阳耀斑爆发活动所引起的地磁扰动的发生及Ap指数进行了预报,取得了较好的结果. 相似文献
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M. K. Reuss E. Keppler M. Fränz M. Witte N. Krupp B. Wilken A. Balogh R. J. Forsyth X. Moussas J. M. Polygiannakis A. D. Kakouris A. Alevizos 《Space Science Reviews》1995,72(1-2):343-346
In November 1992, the Ulysses spacecraft observed a multiple solar particle event and a CME event at 5.2 AU and a heliographic latitude of 20° S which were superimposed to the recurrent corotating interacting region. Distinct particle flux increases caused by these events were observed in all energy channels of the EPAC experiment. The experimental findings are discussed. 相似文献
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通过将燃气空调与传统的电空调器进行对比,指出燃气空调具有能源利用合理、环保、节能高效等优点,并对燃气空调的发展应用进行了展望,认为燃气空调将成为我国未来新型空调的发展方向。 相似文献
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V. Florinski 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
This paper discusses the transport of energetic charged particles through a sectored magnetic field in distant regions of the inner heliosheath. As the plasma flow slows down on approach to the stagnation point on the heliopause, the distance between the folds of the current sheet decreases to the point where it becomes comparable to the cyclotron radius of a cosmic ray particle. Under these conditions a particle can effectively drift across the stack of magnetic sectors with a speed comparable with the particle’s velocity. For a random distribution of current sheet separation distances, a diffusive transport across the stack of sectors occurs instead. The proposed mechanism could have contributed to unusually high intensities of galactic cosmic rays measured by Voyager 1 in the heliosheath during 2009–2010. 相似文献
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L.L. Lazutin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
Temporal variations of the radiation belt particle during the magnetic storms are investigated using measurements by the low altitude satellite spectrometer. Along with several known effects, such as the outer radiation belt intensity decrease at the main phase, the radial diffusion with the particle acceleration and the recovery of the radiation belt during the recovery phase, some less known features were investigated, such as the dawn–dusk asymmetry of the radiation belt. 相似文献
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基于嫦娥一号高能粒子数据的地球磁层屏蔽效应研究 总被引:1,自引:0,他引:1
月球绕地球运行轨道约有1/4位于地球磁层内,因此,地球磁层是否会为月球轨道附近高能粒子提供足够的磁场屏蔽对于探索月球活动具有重要影响.嫦娥一号是中国首颗绕月人造卫星,其绕月飞行的工作轨道距离月球表面200 km.通过对嫦娥一号高能粒子探测器(HPD)的探测数据进行分析,比较了当月球位于地球磁层内外6个不同能道(能量范围4~400 MeV)时质子通量的变化,发现当月球位于地球磁层内时,这些能道的质子通量并没有发生显著减少,结果表明地球磁层不能为月球轨道附近高能粒子提供显著的磁屏蔽. 相似文献