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881.
本文指出现有亚暴的中性线模型其源区在赤疲乏面上离地球太远;以GEOS-2的观测资料为依据,提出了亚暴膨胀相的一个近地触发模型-气球模不稳定性模型,该模型认为,在增长相期间到达R≈(6-10)RE的近地等离子体片内边缘区,出现指向地球方向的离子压强梯度,越尾电流强度增大,磁力线向磁尾拉伸。当等离子体片变薄,电子沉降增强,极光带电离层电导率骤增时,气球模不稳定性在近地等离子体片内边缘区被激发,场向电流 相似文献
882.
Long-term survival of bacterial spores in space. 总被引:8,自引:0,他引:8
G Horneck H Bucker G Reitz 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1994,14(10):41-45
On board of the NASA Long Duration Exposure Facility (LDEF), spores of Bacillus subtilis in monolayers (10(6)/sample) or multilayers (10(8)/sample) were exposed to the space environment for nearly six years and their survival was analyzed after retrieval. The response to space parameters, such as vacuum (10(-6) Pa), solar electromagnetic radiation up to the highly energetic vacuum-ultraviolet range (10(9) J/m2) and/or cosmic radiation (4.8 Gy), was studied and compared to the results of a simultaneously running ground control experiment. If shielded against solar ultraviolet (UV)-radiation, up to 80 % of spores in multilayers survive in space. Solar UV-radiation, being the most deleterious parameter of space, reduces survival by 4 orders of magnitude or more. However, up to 10(4) viable spores were still recovered, even in completely unprotected samples. Substances, such as glucose or buffer salts serve as chemical protectants. With this 6 year study in space, experimental data are provided to the discussion on the likelihood of "Panspermia". 相似文献
883.
884.
M.O. Riazantseva G.N. Zastenker J.D. Richardson 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,35(12):2147-2151
We investigate properties of large (>20%) and sharp (<10 min) solar wind ion flux changes using INTERBALL-1 and WIND plasma and magnetic field measurements from 1996 to 1999. These ion flux changes are the boundaries of small-scale and middle-scale solar wind structures. We describe the behavior of the solar wind velocity, temperature and interplanetary magnetic field (IMF) during these sudden flux changes. Many of the largest ion flux changes occur during periods when the solar wind velocity is nearly constant, so these are mainly plasma density changes. The IMF magnitude and direction changes at these events can be either large or small. For about 55% of the ion flux changes, the sum of the thermal and magnetic pressure are in balance across the boundary. In many of the other cases, the thermal pressure change is significantly more than the magnetic pressure change. We also attempted to classify the types of discontinuities observed. 相似文献
885.
G. Brner E. Seiler 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
The picture of an exponentially increasing, “inflationary” phase of the early universe (Guth 1981; Linde 1982; Albrecht and Steinhardt 1982) may point the way to an understanding of our present universe without reference to extremely specific initial conditions. The model rests, however, on several assumptions which deserve critical examination. 相似文献
886.
大型转动机械碰摩故障分析的声发射检测系统 总被引:5,自引:0,他引:5
吴建 《北京航空航天大学学报》1998,24(1):104-107
汽轮发电机、空气压缩机等采用油膜支撑的大型转动机械,由于安装或运行中的原因,在转子旋转过程中,可能和器壁发生轻微的摩擦和碰击,简称碰摩.声发射技术在碰摩发生特别是故障早期诊断上有优越性.本系统的特点是没有沿用传统的计数、幅度、能量和持续时间等声发射特性参数,而是在声发射包络信号的频率分析中进行特征提取.声发射发生的过程分析和现场试验都表明这种方法对碰摩检测很敏感,在碰摩发生的起始阶段,包络谱中与转速同步的周期性分量显著增加.根据这种新的设计思想自行研制了BUAA碰摩声发射检测仪并对此作了介绍. 相似文献
887.
拉形条件对镜面蒙皮成形质量的影响 总被引:4,自引:2,他引:4
万敏 《北京航空航天大学学报》1998,24(6):654-657
在充分考虑滑移带出现与成形件贴模度的基础上,通过分析拉形速度、毛料几何尺寸、模具几何参数、润滑方式对成形质量的影响,确定了合理的飞机镜面蒙皮拉形条件.结果表明,改善板料变形的均匀性,延缓滑移带出现,增加成形面内材料的变形程度,是制定最优工艺参数、提高成形质量的主要措施. 相似文献
888.
冗余度机器人力控制的运动学稳定性分析 总被引:1,自引:0,他引:1
把非冗余度机器人位置/力混合控制方案引入到冗余度机器人,用线性化的动力学模型对其运动学稳定性进行分析,提出一种改进的基于运动学稳定的冗余度机器人混合控制策略。仿真研究结果证明了所提出方法的有效性。 相似文献
889.
T.L. Zhang H. Zhao C.T. Russell S.M. Petrinec K. Schwingenschun W. Riedler 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1997,19(12):1943-1946
The northward and southward orientation of the interplanetary magnetic field (IMF) is usually considered as providing the external boundary conditions in the solar wind interaction with the Earth's magnetopause but it is the magnetic field in the magnetosheath that interacts with the Earth's magnetic field. In this paper, we consider the possibility that the wave activity in the foreshock region may affect the magnetic field orientation in the magnetosheath with time scales that might be geomagnetically effective. If magnetosheath magnetic field becomes disturbed on plasma streamlines which are connected to the quasi-parallel bow shock and foreshock, the magnetic field orientation on the inner magnetosheath may differ significantly from the undisturbed IMF. We present a model of dayside reconnection which may occur when the IMF northward and illustrate its effects on the erosion of the magnetopause. 相似文献
890.
D Voeste L H Levine H G Levine V Blum 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2003,31(1):211-214
The Closed Equilibrated Biological Aquatic System (C.E.B.A.S.) Mini-Module, a Space Shuttle middeck locker payload which supports a variety of aquatic inhabitants (fish, snails, plants and bacteria) in an enclosed 8.6 L chamber, was tested for its biological stability in microgravity. The aquatic plant, Ceratophyllum demersum L., was critical for the vitality and functioning of this artificial mini-ecosystem. Its photosynthetic pigment concentrations were of interest due to their light harvesting and protective functions. "Post-flight" chlorophyll and carotenoid concentrations within Ceratophyllum apical segments were directly related to the quantities of light received in the experiments, with microgravity exposure (STS-89) failing to account for any significant deviation from ground control studies. 相似文献