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锂离子电池在社会生产各领域应用广泛,由于其复杂的电化学系统,状态检测难度较大,给供电保障带来不利影响.结合Thevenin等效电路与中心差分卡尔曼滤波法(CDKF),构建了一种聚合物锂离子电池的荷电状态(SOC)估计模型.MATLAB仿真验证表明,该模型能有效防止安时计数误差累积,电池SOC估计误差不超过5%. 相似文献
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分别利用大气等离子喷涂技术制备了Ni/Al粘结底层、火焰喷涂技术制备了NiCrAl/Diatomite可磨耗封严涂层,研究了喷涂距离、送粉速率、火焰气体总流量、喷涂角度和氧燃比等喷涂参数对生长速率和涂层硬度的影响。结果表明,在较低的氧燃比条件下(O2∶C2H2<1.6),随着喷涂距离的增大,涂层生长速率逐渐下降,硬度先保持不变后逐渐上升;当O2∶C2H2>1.6时,涂层的生长速率会随着喷涂距离的增大先增大后减小,硬度随之逐渐下降。随着喷枪对基体相对移动速度的增大,涂层生长速率略微下降,硬度略有上升。气体总流量的增大使得涂层的生长速率明显上升,硬度明显下降。随着送粉量的增大,涂层生长速率明显提高,硬度随之先上升后下降。 相似文献
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To obtain high-quality aviation forgings of titanium alloys, b forging is an essential processing step which must be considered throughout a production process. In this work, the effect of b forging on the crystal orientation and morphology of lamellar a was experimentally investigated in a two-phase titanium alloy. Strong dynamic recovery during b working resulted in the formation of low-angle grain boundary(LAGBb) inside b grains. The lamellar a can penetrate through the LAGBb, leading to similar intra a LAGBs on subgrain boundaries. Deformation banding occurs at high strain rates, and both diffusive and sharp boundaries of deformation bands can be observed.A continuous change of the b orientation in diffusive boundaries results in the formation of fine and disordered a lamellae without intra-lamellar boundary to hold the Burgers orientation relationship(OR). On sharp boundaries, it is prone to producing continuous grain boundary a(aGB) with a highly similar orientation along the boundaries. Meanwhile, there may exist several lower-angle boundaries within the grain boundary a for a smoother orientation change on the b grain boundary. 相似文献
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Jia Luo Fangfang Sun Xiaohua Xu Han Wang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(1):327-336
In this paper, we compared the F2-Layer critical frequency (foF2) derived from FORMOSAT-3/COSMIC radio occultation (RO) and ionosondes at Chiang Mai, Chumphon and Kototabang during the years 2008–2015 to evaluate the performance of COSMIC RO over Southeast Asia region. The results show that the time development of foF2 values derived from COSMIC RO generally agrees well with those from ionosonde measurements. However, the differences between the foF2 derived from COSMIC RO and that derived from ionosonde observations display latitudinal dependence. COSMIC RO tends to underestimate foF2 at Chiang Mai and Kototabang, which is near to the north EIA crest and the south one, respectively, while a little overestimate foF2 at Chumphon, which is close to the geomagnetic equator. COSMIC RO agrees best with ionosonde at Chumphon and worst at Chiang Mai. At each ionosonde station, the quality of COSMIC RO data degrades with the increase of solar activity. In addition, at the station Chiang Mai and Kototabang, COSMIC RO performs better in summer than in equinox and winter. Furthermore, the differences in foF2 derived from COSMIC RO and that from ionosonde measurements vary with local time, i.e., the differences in foF2 are generally smaller at night and larger in noontime when equatorial ionization anomaly (EIA) is well developed. 相似文献
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Rui Tu Jinhai Liu Rui Zhang Pengfei Zhang Xiaodong Huang Xiaochun Lu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(2):913-926
This paper proposes a real-time kinematic (RTK) model that uses one common reference satellite for the Galileo system with four frequency observations. In the proposed model, the double-differenced (DD) pseudorange and carrier phase biases among the different frequencies are estimated as unknown parameters to recover the integer features of the DD ambiguities among the different frequencies for ambiguity resolution and precise positioning. Analysis results show that the E5a, E5b, and E5 frequencies have virtually the same performance in terms of the positioning accuracy, observation residuals, and ratio values of ambiguity resolution. However, the E1 frequency performs worse than the E5a, E5b, and E5 frequencies. The RTK results for the combination of multiple frequencies are much better than those for a single-frequency observation, the coordinates’ standard deviation is improved about 20–30%, and the ambiguity fix time is improved about 10%. 相似文献
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Aiming at the challenges caused by the persistence, concurrency and energy consumption of probe actions, a plan repair method of deep space probe based on the expected state sequence is proposed. In this method, the expected state sequence is formed of the expected effect of the unfinished action and the expected precondition of the unexecuted action in the pre designed plan, according to the execution status of the action. The expected state sequence is an ordered set of states with mixed logic and energy, providing subgoals for plan repair and also transforming the plan repair problem into the state transition path searching problem. During the search, the plan repair strategy with energy supply priority is proposed, which separates the logic repair from energy repair to reduce the difficulty of solving the problem. And this method enables the probe to recover from plan failure autonomously. Finally, the effectiveness and rationality of the proposed method are verified through simulation by taking the Mars Orbiter as an example. 相似文献
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针对高超声速飞行器三通道具有强耦合的问题,提出一种基于扩张状态观测器的全通道解耦控制方法。该方法不需要根据耦合项特点设计耦合补偿模型,而是通过设计扩张状态观测器,将高超声速飞行器耦合项视为扰动,利用扩张状态观测器具有实时跟踪估计扰动的能力,将耦合项扰动估计出来。通过补偿控制来消除耦合的影响,从而完成解耦控制。进一步,通过LQR控制方法完成姿态控制系统的闭环反馈控制律设计,最终实现一种工程上实用的高超声速飞行器解耦控制方法,并通过数学仿真验证了该控制方法的正确性和有效性。 相似文献