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要成功地发射一个深空探测器进入目标轨道,相应的运行过程基本上涉及3个阶段:近地停泊轨道运行段、转移轨道的过渡段和进入目标天体的绕飞段。它们各自的运行状态和相应的数学模型有所差别,特别是转移轨道段的运行特征与绕飞段的卫星轨道的典型特征之间的重大差别,在深空探测任务中受到广泛的重视,如平动点利用中的晕(Halo)轨道和引力加速的节能过渡等。然而,就太阳系而言,这些不同轨道之间有一共同的基本性态,那就是都可以用在牛顿万有引力定律制约下的开普勒轨道(或变化的开普勒轨道)来刻画。本文将针对上述不同运行段轨道对应的数学模型、研究方法和结果,结合我们所做的工作进行综述。 相似文献
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B. Kirov K. Georgieva D. Batchvarov A. Boneva R. Krasteva G. Stainov S. Klimov T. Dachev 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
The main purposes of experiment “Obstanovka” (“Environment” in Russian) consisting of several instruments are to measure a set of electromagnetic and plasma phenomena characterizing the space weather conditions, and to evaluate how such a big and highly energy consuming body as the International Space Station disturbs the surrounding plasma, and how the station itself is charged due to the operation of so many instruments, solar batteries, life supporting devices, etc. Two identical Langmuir electrostatic probes are included in the experiment “Obstanovka”. In this paper the Langmuir probes for “Obstanovka” experiment are described, including the choice of geometry (spherical or cylindrical), a more reliable method for the sweep voltage generation, an adaptive algorithm for the probe’s operation. Special attention is paid to the possibility for remote upgrading of the instrument from the ground using the standard communication channels. 相似文献
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针对带探针装置的倾斜卧式椭直圆筒罐罐容表函数(即罐内储油量与探针油位高度对应的函数关系)的理论计算问题,首先采用"冰冻"思维和相对运动等效地把倾斜卧式的情形转化为水平卧式的情形,然后根据液面与关键液面的不同位置关系采取了不同的计算方法,最后分段地得到了罐容表函数的一般表达式。 相似文献
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参考了近40年来国外有关超音速和高超音速静压探针的研究成果,设计了多种并发展了二种高超音速静压探针。它们可精确地用于持续工作流场仅为30ms的流场静压测量。实测静压与自由流静压比p_(s,m)/p_(s,∞)=1.009;马赫数比M_(∞m)/M_(∞,)=0.993。实验在加拿大多伦多大学宇航研究院的高超音速炮风洞里完成。炮风洞喷管出口气流特性是:(空气)自由流总压比_(t,∞)=25.5MPa,总温T_(t,∞)=1000K;马赫数M_∞=8.30;自由流静压p_(s,∞)=2.13kPa;雷诺数R_e=3.2×10~7。以探针直径D为基准的R_(e,D)=34,000~52,800。这种探针己被用于“管内高超音速流场发展实验研究”中了。 相似文献
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Valentin A. Shuvalov Dmitry N. Lazuchenkov Nikolai B. Gorev Galina S. Kochubei 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(1):355-366
Using a cylindrical Langmuir probe and the authors’ proprietary two-channel pressure transducer, ionospheric plasma parameter distributions along the orbit of the Sich-2 satellite (Ukraine, 2011–2012) were measured. This paper is concerned with identifying the space–time location of ionospheric plasma disturbance sources, including the epicenters of actual earthquakes (before or during the satellite flyover) and incipient earthquakes on the subsatellite track, from the measured distributions of the electron density and temperature and the neutral particle temperature along the satellite orbit. To do this, the measured ionospheric plasma parameter distributions are connected to the coordinates on the subsatellite track.It is shown that local disturbances in the electron density and temperature and neutral particle temperature distributions in the satellite orbit in the ionosphere may serve as indicators of seismic activity on the subsatellite track. The epicenters of incipient earthquakes may be set off from other plasma parameter disturbance sources associated with seismic activity using information provided by special monitoring and survey centers that monitor the current seismic situation. 相似文献
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Lei ZU Xianzhao XIA Qian ZHANG Xiaolong JIA Huabi WANG Guiming ZHANG Jinhu LU 《中国航空学报》2022,35(4):438-449
This paper tested the viscosity of prepreg in the automatic placement process, and conducted the probe and placement-90° peel tests through the test systems. The law of variation of prepreg viscosity during the laying process was studied through these tests under different conditions by taking the peel force to intuitively and quantitatively characterise the viscosity of the prepreg.The results show that this viscosity is inversely proportional to the laying rate, proportional to the laying pres... 相似文献
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《中国航空学报》2016,(2):448-461
In a probe and drogue aerial refueling system, the bow wave of the receiver aircraft will produce a strong aerodynamic effect on the drogue once the receiver follows the drogue at a close distance. It is a major difficulty of docking control in the probe and drogue refueling. This paper analyses the bow wave effect and presents a simple method to model it. Firstly, the inviscid flow around the receiver is modeled based on the stream function defined by basic stream singularities.Secondly, a correction function is developed to eliminate the error caused by the absence of air viscosity. Then, the aerodynamic coefficients are used to calculate the induced aerodynamic force on the drogue. The obtained model is in an analytical form that can be easily applied to the controller design and the real-time simulations. In the verification part, computational fluid dynamics(CFD)simulation tests are conducted to validate the obtained flow fields and aerodynamic forces. Finally,the modeling method is applied to an F-16 receiver aircraft in a previously developed autonomous aerial refueling simulation system. The simulations results are analyzed and compared with the NASA flight-test data, which demonstrates the effectiveness of the proposed method. 相似文献