数控加工中在线测量线轮廓度误差应用研究

探讨数控加工中利用误差分离技术在线测量线轮廓度误差新方法,在进行误差分离计算机仿真基础上,在实际加工中进行实测,测量准确度和测量效率大大提高.     

Analysis of the code and phase between-receiver inter-system biases of the overlapping frequencies for GPS/Galileo/BDS

The overlapping-frequency signals from different GNSS constellations are interoperable and can be integrated as one constellation in multi-GNSS positioning when inter-system bias (ISB) is properly disposed. The look-up table method for ISB calibration can enhance the model strength, maximize the number of integer-estimable ambiguities, and thus is preferred. However, the characteristics and magnitudes of the receiver code ISB and phase fractional ISB (F-ISB) are not well known and the wrong values of the biases can seriously degrade the positioning results. In this contribution, we first estimate the between-receiver code ISB and phase F-ISB of hundreds of the baselines up to around 25km in the European Permanent GNSS Network (EPN) and the Multi-GNSS Experiment (MGEX) for the overlapping frequencies L1-E1 (L1), L5-E5a (L5) and E5b-B2b (L7). The data collected from 1st January 2016 to 1st January 2019. Second, the receiver-type and firmware-version combinations for the receivers of Trimble, Leica, Javad, Septentrio and NovAtel are carefully classified. Results show that the Septentrio receivers have consistent code and phase ISB values for the three overlapping frequencies i.e. only one value for each frequency and no receivers are different. The Leica, Trimble and Javad receivers have two or more ISB values for at least one of the three frequencies. A few receivers with biases to the groups are also found and listed. Third, the code ISB and phase F-ISB of the groups are adjusted by the least-squares method. The root mean square errors (RMSE) of the least square adjustment are 0.240 m, 0.250 m and 0.200 m for code of L1, L5 and L7 frequencies, respectively, and are 0.0009 m, 0.0015 m and 0.0031 m for phase of L1, L5 and L7 frequencies, respectively. Finally, the effects of code ISB errors on code positing are investigated with the zero-baseline MAT1_MATZ. The distance root mean square error (DRMS) of L1-E1 code positioning can be reduced by 48.2% with 5 GPS and Galileo satellites and the DRMS degrades quickly when the code ISB error is larger.     

基于最小熵准则的频偏估计算法研究

提出了一种基于SEM(Spectrum Entropy Minimization,频谱熵最小化)的频偏估计算法。研究发现,频偏越小,离散信号频谱的熵越小。根据这一性质建立了相关算法,通过一维搜索的方式得到使相位补偿后信号频谱熵最小的频偏估计。仿真结果表明:SEM算法的估计性能能够达到CR(Cramer-Rao,克拉美罗)下界,而且估计的稳定性和鲁棒性较好,具有一定的应用价值。     

Modeling the coronal magnetic field in a polar hole

The coronal magnetic field in the northern polar coronal hole in 1986 is predicted on the basis of the photospheric magnetic field observations and the horizontal current-current sheet coronal model (Zhao and Hoeksema, 1993). The predicted magnetic field intensity is stronger near the center of the hole than near the edge. The calculated expansion factor for the entire hole does not match the expansion factor of any flux tube in the hole, suggesting that it would not be appropriate to use the expansion factor for entire hole to represent the divergence of the flux tube in analyzing the acceleration and heating of the plasma in coronal holes.     

连续分离铝熔体中夹杂物的分析

通过分析高频磁场作用下熔体连续处理时夹杂的去除效率表明，熔体连续处理条件下的夹杂去除效率比熔体静止时的略低，而夹杂与熔体之间的密度差对电磁分离时的去除效率影响不大。提高去除效率的有效途径是增大磁感应强度或降低分离器管径，但减小管径的同时需要提高磁场频率，以保持α/δ的值在2附近才可以取得最佳的分离效果。     

超燃冲压发动机带凹槽的燃烧室流场振荡研究

为了分析闭式凹槽的流场振荡现象,结合试验和二维非定常数值模拟方法,开展了三种条件下的非定常研究.通过实验发现,长深比较大的凹槽作为超燃冲压发动机火焰稳定装置时,凹槽的冷流流场存在强烈的振荡现象.结合二维非定常数值模拟方法,初步分析了振荡机理:振荡的主要原因是燃烧室入口气流马赫数的大小,马赫数2.0条件下,流场周期振荡;马赫数3.0条件下,流场可以稳定存在.根据分析结果给出了流场特征与马赫数的定性依赖关系.通过增加隔离段长度的方法对分析结果进行了验证.     

中国股票市场中的现状偏好现象研究

理性人假设历来饱受诟病,现状偏好现象在成熟资本市场广泛存在.西方行为金融学学者提出了现状偏好理论,而该理论在我国鲜有实证支持.尝试提出了以中国股票市场的正负收益率对换手率的不对称影响来衡量现状偏好现象的理论,选择了我国2011年1月4日至2012年9月28日之间上交所和深交所挂牌的主板A股的数据进行实证分析,发现中国股票市场存在明显的现状偏好现象,并计算出该时期上交所主板A股的现状偏好系数为9.61％,上交所主板A股的现状偏好系数为11.11％.     

精密卫星钟差分形插值算法研究

研究发现精密GPS卫星钟差时序满足三阶平稳假设,由此提出了计算卫星钟差分形维的多阶分形变差法,进而提出了基于分形维确定垂直比例因子的精密卫星钟差分形插值算法。将新方法应用于2010年8个节气日的32颗GPS在轨卫星钟差分形维计算,并选取Block IIA、IIR和IIR\|M各2颗卫星进行钟差插值精度比较。结果表明,分形维可作为定量描述卫星钟差动力学特征的不变量指标;分形插值算法优于三次样条和切比雪夫算法,可以满足快速与高采样率精密卫星钟差应用需求。     

Effect of the Interplanetary Electric Field on the Magnetopause From Global MHD Simulations

The north-south component B_z of the Interplanetary Magnetic Field (IMF) and solar wind dynamic pressure P_d are generally treated as the two main factors in the solar wind that determine the geometry of the magnetosphere. By using the 3D global MHD simulations, we investigate the effect of the Interplanetary Electric Field (IEF) on the size and shape of magnetopause quantitatively. Our numerical experiments confirm that the geometry of the magnetopause are mainly determined by P_dB_z, as expected. However, the dawn-dusk IEFs have great impact on the magnetopause erosion because of the magnetic reconnection, thus affecting the size and shape of the magnetopause. Higher solar wind speed with the same B_z will lead to bigger dawn-dusk IEFs, which means the higher reconnection rate, and then results in more magnetic flux removal from the dayside. Consequently, the dayside magnetopause moves inward and flank magnetopause moves outward.      

新型磁流变减摆器节流孔流场分析

节流孔是磁流变减摆器产生阻尼的主要方式,在磁流变减摆器实际工作环境下,磁流变液经过磁场时会随磁场分布强度不同而产生变黏度等应激变化。建立某新型磁流变减摆器计算模型,通过改变节流孔孔径大小,使用商业软件 Fluent 对其所产生的流场进行分析,将模拟结果与实验结果进行对比。结果表明:磁流变液流通量及淤积效应是决定磁流变减摆器初始阻尼及时滞效应的主要原因;在 0.2mm 孔径时时滞效应最明显,且随频率增高磁流变减摆器对于外界激励反应速度明显下降。