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961.
962.
在丁羟/铝粉/高氯酸铵组成的三组元推进剂体系中,通过药浆流变性测试、动态力学分析(DMA)、单向拉伸性能、凝胶分数和相对交联密度的测定,研究了一些功能组分如氮丙啶类化合物MAPO、醇胺络合物TEA·BF3、胺类化合物H对推进剂工艺性能和力学性能的影响.结果表明,MAPO可以降低药浆屈服值和表观粘度,改善工艺性能,显著增加最大抗拉强度,但对最大伸长率无影响;TEA·BF3大幅度增加药浆屈服值,使工艺性能变差,一定程度上提高最大抗拉强度和发挥熵弹性而增加最大伸长率,H可以显著改善推进剂工艺性能和增加最大伸长率.文中还对功能组分在推进剂中的作用机理进行了分析探讨. 相似文献
963.
丁羟推进剂粘合剂网络结构调控方法探讨 总被引:4,自引:2,他引:4
把扩链剂的使用作为调整丁羟推进剂粘合剂网络及其形态结构的一个重要手段。采用扩链剂、交联剂和真实固化参数(Rt)等综合的方法调控丁羟推进剂性能,可望比单纯控制名义固化参数(Ro)获得更好的力学性能及其稳定性。推导了丁羟推进剂粘合剂系统网络调整的通用计算公式和各种特定条件下的计算公式。 相似文献
964.
Determination of the Microacceleration Quasisteady Component onboard the International Space Station
Babkin E. V. Belyaev M. Yu. Efimov N. I. Sazonov V. V. Stazhkov V. M. 《Cosmic Research》2004,42(2):155-164
A comparison of two methods of determination of the microacceleration quasisteady component arising onboard the International Space Station was performed. In the first method the acceleration was calculated using the relative motion of the station reconstructed on the basis of telemetry data. The second method was a direct measurement of the microacceleration by a low-frequency accelerometer and a smoothing of the data obtained. The used measurements were made by the American accelerometer MAMS. The above comparison can theoretically be used to refine the position of the station center of mass relative to its body. 相似文献
965.
Eiges P. E. Zastenker G. N. Safrankova J. Nemecek Z. Eismont N. A. 《Cosmic Research》2001,39(5):432-438
Based on simultaneous measurements of ion fluxes made onboard the closely separated satellites Interball-1and Magion-4, the propagation velocity of middle-scale plasma structures in the Earth's foreshock relative to the solar wind flow is estimated. The derived value of this velocity allows these structures to be identified as a fast magnetosonic wave propagating upstream of the solar wind inflowing the Earth's bow shock. An evaluation is also made of the correlation length of these disturbances in the plane perpendicular to the Sun–Earth line. This length is approximately equal to 2R
E. 相似文献
966.
967.
968.
Zetzer J. I. Kozlov S. I. Rybakov V. A. Ponomarenko A. V. Smirnova N. V. Romanovsky Yu. A. Meng C.-I. Erlandson R. Stoyanov B. 《Cosmic Research》2002,40(3):233-240
The measurements of infrared emission from an artificial structure, which was generated during the Fluxus experiment with plasma jet injection into the atmosphere, are obtained and discussed for the first time. Additional experimental data on the airglow in the visible spectral band of the disturbed region of the atmosphere are presented. A generalized analysis of the data is given. 相似文献
969.
G. L. Gdalevich N. I. Izhovkina V. D. Ozerov N. Bankov S. Chapkanov L. Todorieva 《Cosmic Research》2006,44(5):419-424
The results of the satellite low-latitude and mid-latitude measurements of the disturbed plasma concentration, electron temperature, and quasi-stable electric field at heights of ~900 km after sunset are discussed. It is shown that the sharp fronts of changes in the electron temperature and plasma density observed in the experiment onboard the Intercosmos-Bulgaria-1300 satellite in the low-latitude (and equatorial) outer ionosphere can be related to damping of the oscillations of plasma electrons at local decreases of the plasma density (plasma “pits”) and formation of the vortex plasma structures at density and temperature gradients, which promotes conservation of ionosphere irregularities and makes the fronts of concentration variations steeper. Nonmonotonic variations in the plasma conductivity for the ionosphere currents in unstable plasma can be a cause of observed nonmonotonic disturbances of the vertical component of the “constant” electric field. 相似文献
970.
Ali G. Hafez Essam Ghamry 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
One of global processes in ionosphere–thermosphere–magnetosphere system is the geomagnetic storms. It is of great importance to develop an algorithm that auto-detects sudden commencement because it could be an indicator of onset of the geomagnetic storm. Automatic detection of geomagnetic sudden commencement is based on time–frequency clusters generated by spectrogram. Proposed algorithm is tested on data set collected from stations belong to the international real-time magnetic observatory network (INTERMAGNET). Maximum standard deviation of algorithm detection times is observed to be one minute of the corresponding arrival times published by National Geophysical Data Center (NGDC). 相似文献