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201.
V.M. Sorokin O.A. Pokhotelov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The influence of quasi-static electric field of seismic origin on the characteristics of the internal gravity waves (IGWs) in the Earth’s ionosphere is considered. The electric field in the ionosphere arises due to the injection of charged aerosols into the atmosphere, formation of an EMF in the near Earth atmosphere and perturbation of the conductive electric current in the global electric circuit. Amplification of the electric current in seismic zone is accompanied by the formation of perturbation of the lower ionosphere that affects the amplitude and phase of VLF/LF signals. The action of the electric field on the IGWs is connected with the appearance of the Ampere’s force in the ionosphere. In the spectral range of these waves the latter acts on the neutral component of the ionosphere plasma. As the result of this interaction the ionosphere starts to support the discrete spectrum of oscillations. Periods of their maximums increase as numbers of natural sequence. The existence of such peculiarities of the waves in the ionosphere is confirmed by observations. 相似文献
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204.
改善离子推力器束流均匀性的方法 总被引:5,自引:5,他引:0
离子推力器的束流分布,直接影响离子推力器离子光学系统(亦称栅极组件)的性能和寿命。通过对离子推力器离子光学系统的改进和放电室磁场的优化,使束流均匀性系数R值达到0.7左右。离子推力器束流分布均匀性的有效提高,有助于改善离子光学系统的受热分布,降低离子光学系统的温度,并能减小其温度差,使离子光学系统的热应力和热变形降低,进而延长离子推力器的寿命。 相似文献
205.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2023,71(1):1137-1145
The relationship of auroral activity indices (AE, Kp, SME) with interplanetary medium parameters during the main phase of magnetic storms is studied. For the period 1990–2020, 142 magnetic storms driven by (41) Sheath, (61) CIR, and (40) ICME events are selected. It is found that the correlation coefficient between average values of the SME index and the SW electric field for Sheath (r = 0.75) is close to correlation coefficients for CIR and ICME events. The correlation coefficient between Kpaver&Eswaver (r = 0.72) is higher than the correlation coefficient between AEaver&Eswaver (r = 0.63) at the main phase of magnetic storms induced by the Sheath events. It is shown that average values of SW dynamic pressure and IMF σB fluctuations correlate each other for all types of SW. 相似文献
206.
C. Rioux R.J. Slobodrian 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
The aggregates formed in low gravity are generally fractals. The fractal dimensions and the site growth probability measures of the resulting fractal structures strongly depend on the properties of the forces that cause the aggregation. Using some approximations, we solved the equation of motion and obtained the relation giving the particles separation as a function of time. The electric force between two charged particles and the magnetic force between two particles with a magnetic moment were considered. The two relations are different and it is shown that one can identify and separate these two interactions by analysing the recording of the aggregation. The apparatus used to record the aggregation has a resolution in the order of one micrometer per pixel and has the possibility of recording simultaneously two views at right angles. From a three dimensional recording of an aggregation, it will be possible to obtain the product of the two charges or magnetic moments causing the aggregation. 相似文献
207.
208.
离子推进及其关键技术 总被引:1,自引:1,他引:1
介绍离子式电推进的工作原理、性能参数、发展历史和现状。阐述了发展离子推进需攻克的关键技术,其中包括提高性能(比冲、推力、工质利用率等)、延长工作寿命、与卫星的相容性、离子光学系统等。 相似文献
209.
基于H∞滤波的GPS/INS全深组合导航系统研究 总被引:5,自引:0,他引:5
根据H∞鲁棒滤波理论,提出了基于H∞滤波技术的GPS/INS全深组合导航系统,该系统仅含有位置误差,速度误差和平台误差角9维状态,并利用伪距,伪距率和载波相位观测信息对全部状态进行观测,组成全深组合导航系统,由H∞滤波来提高系统的鲁棒性,文中对提出的组合系统了动态仿真,仿真结果表明,该系统结构简单,状态估计精工高,系统鲁棒性好,便于工程实现。 相似文献
210.
Baolin Tan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2007,39(12):1826-1830
The distributing profile of electric current in solar plasma loop is a key factor for the MHD instabilities of the loops. However, it is very difficult to measure such profile in single loop. In this paper, we assume that, in spite of the complexity of the structure in most of the sunspots, the distribution of the electric current in some small simple sunspots may reflect the main feature of the distribution in solar plasma loops. We utilize the high-cadence, high-resolution vector magnetograms observed by Big Bear Solar Observatory (BBSO) to derive the longitudinal electric current and analyze the distribution of the longitudinal electric current in the region of sunspots, and simulate the distributing features of the solar plasma loops. From these analysis, we find that the electric current in some small simple sunspots, or to say in plasma loops, are concentrated to their center. Such distribution feature is consistent with the theory of pinch effect in current-carrying plasma loops. 相似文献