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针对半球谐振陀螺的零位漂移问题,本文研究了基于模态反转电路控制技术的零位自校准方法。首先,从动力学模型引入阻尼不对称、频率裂解等非理想因素,讨论半球谐振陀螺的工作机理及驻波漂移特性。其次,通过理论分析模态反转的零位校准以及虚拟进动控制的模态反转技术。最后,基于FPGA数字控制平台,设计并实现了半球谐振陀螺零位自校准半实物仿真实验。实验结果表明,基于模态反转的半球谐振陀螺零位校准,实现了半球谐振陀螺的零位从15 降低至2 ,短期零偏稳定性和长期稳定性也分别提高了11.8%和45.86%,有效地抑制了零位漂移,提高了半球谐振陀螺测量精度。 相似文献
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《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(5):1619-1633
The behaviour of the equatorial/low-latitude ionosphere and the transport processes during magnetic disturbed and quiet periods of a high solar activity year, 2014, in the American sector are investigated. Parameters used include vertical drift (Vz), transport term (W), NmF2, hmF2 and scale-height (H). The F2 plasma variations followed the diurnal local solar pattern, being higher at daytime. The sunset maximum and sunrise minimum peaks of hmF2 were directly opposite to the scale height (H) pattern. The plasma distribution was basically controlled by combined actions of the electrodynamic convection/thermospheric composition, which is geomagnetic activity dependent. The annual, semi-annual and winter-anomalies of the F2 parameters were higher at the dip equator in comparison with the low-latitude. The Vz pre-reversal peak magnitude coincided with hmF2 peak and the effects are more pronounced during geomagnetic disturbed conditions. The transport term pattern was similar to that of the scale height and it is suggested as a proxy parameter for quantifying low-latitude plasma irregularities and distribution of thermospheric composition. 相似文献
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Qiang Guo Volodymyr G. Galushko Andriy V. Zalizovski Sergiy B. Kashcheyev Yu Zheng 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(9):2267-2274
A modification of the Doppler Interferometry Technique is suggested to enable estimating angles of arrival of comparatively broadband HF signals scattered by random irregularities of the ionospheric plasma with the use of small-size weakly directional antennas. The technique is based on the measurements of cross-spectra phases of the probe radiation recorded at least in three spatially separated points. The developed algorithm has been used to investigate the angular and frequency-time characteristics of HF signals propagating at frequencies above the maximum usable one (MUF) for the direct radio path Moscow-Kharkiv. The received signal spectra show presence of three families of spatial components attributed, respectively, to scattering by plasma irregularities near the middle point of the radio path, ground backscatter signals and scattering of the sounding signals by the intense plasma turbulence associated with auroral activations. It has been shown that the regions responsible for the formation of the third family components are located well inside the auroral oval. The drift velocity and direction of the auroral ionosphere plasma have been determined. The obtained estimates are consistent with the classical conception of the ionospheric plasma convection at high latitudes and do not contradict the results of investigations of the auroral ionosphere dynamics using the SuperDARN network. 相似文献
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获取高精度事后姿态数据是提高遥感平台成像质量的必要条件之一,离线处理可有效降低敏感器测量误差,从而获得更高的姿态确定精度。基于滤波的校正方法中,星敏感器低频误差(LFE)与陀螺漂移将产生耦合影响导致校正精度低,本文针对该问题推导了耦合误差的数学模型,并设计了一种两步双向平滑事后处理算法,将陀螺漂移与低频误差分两步校正,通过反复滤波剥离陀螺漂移与低频误差。同时,针对低频误差参数收敛速度慢、噪声参数调节困难的问题,利用一种基于极大似然估计(MLE)的固定窗口自适应双向滤波算法进行处理以获得更好的噪声估计,提高了收敛速度和收敛精度。文中仿真工况下,离线姿态确定精度可达到0.8″(3σ),低频误差参数完全收敛时间不超过4个轨道周期。 相似文献
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文章在三维仿真软件HFSS和CST中建立谐振腔模型,给出建模的原理和注意点;详细研究了腔体各尺寸随温度变化对腔体本征频率的影响的正负性及影响大小,得出引起腔体频率变化的主要结构因素;重点分析了调谐螺钉纵向扰动及径向扰动对谐振频率的影响。结合LC谐振电路对结果进行分析,得出减小温漂的措施。并根据仿真结果,对腔体的各个部分合理使用不同材料,使腔体温漂得到补偿。 相似文献
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考虑离子极化漂移中非线性项对动力学Alfven孤波特性的影响,采用双流体模型研究磁化等离子体中低频动力学Alfven稀疏型孤波的特性,所得的结果表明,两种类型的动力学Alfven稀疏型孤波在磁层中大范围内均存在(参数β约为10^-6,0,1,β为等离子体的热压之磁压之比,即β=20μ0nT/B0^2),它们或以超Alfven速或以亚Alfven速传播。同时发现在β值较小(10^-6-10^-4)时,离子极化漂移非线性项对动力学Alfven孤波特性有较大的影响,不可忽略,而在较大值时(β-0.1),此修正作用不大,由于动力学Alfven孤波允许平行电场存在,故它对等离子体中带电粒子的加速和能化起重要作用。同时也对离子的横向加速有一定的作用,它使一种新的能量转换机制成为可能。 相似文献
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