The Qi Tai Telescope(QTT),which has a 110 m aperture,is planned to be the largest scale steerable tele-scope in the world.Ideally,the telescope’s repeated pointing accuracy error should be less than 2.5 arc seconds(a...The Qi Tai Telescope(QTT),which has a 110 m aperture,is planned to be the largest scale steerable tele-scope in the world.Ideally,the telescope’s repeated pointing accuracy error should be less than 2.5 arc seconds(arcsec);thus,the telescope structure must satisfy ultra-high precision requirements.In this pur-suit,the present research envisages a reverse-design method for the track surface to reduce the difficulty of the telescope’s design and manufacture.First,the distribution characteristics of the test data for the track error were verified using the skewness coefficient and kurtosis coefficient methods.According to the distribution characteristics,the azimuth track error was simulated by a two-scale model.The error of the long period and short amplitude was characterized as large-scale and described by a trigonometric function,while the short period and high amplitude error was characterized as small-scale and simulated by a fractal function.Based on the two-scale model,effect of the error on the pointing accuracy was deduced.Subsequently,the relationship between the root mean square(RMS)of the track error and the RMS of the pointing accuracy error of the telescope was deduced.Finally,the allowable RMS value of the track error was derived from the allowable pointing accuracy errors.To validate the effectiveness of the new design method,two typical radio telescopes(the Green Bank Telescope(GBT)and the Large Millimeter Telescope(LMT))were selected as experimental examples.Through comparison,the theoretical calculated values of the pointing accuracy of the telescope were consistent with the measured values,with a maximum error of less than 10%.展开更多
针对自主车辆换道轨迹跟踪精度较低等问题进行了研究。提出了基于轨迹预测的多点预瞄权重增益分配的方法。首先,根据车辆与路径的实时横向偏差以及航向角偏差,建立驾驶员转向模型,获得最优方向盘转角;其次,为了提高车辆换道路径跟踪时...针对自主车辆换道轨迹跟踪精度较低等问题进行了研究。提出了基于轨迹预测的多点预瞄权重增益分配的方法。首先,根据车辆与路径的实时横向偏差以及航向角偏差,建立驾驶员转向模型,获得最优方向盘转角;其次,为了提高车辆换道路径跟踪时的稳定性,采用线性模型预测控制(linear model predictive control,L-MPC)策略设计轨迹跟踪控制器。最后,搭建Carsim&Simulink联合仿真模型,针对不同车速设置对比实验进行分析,结果表明基于轨迹预测的驾驶员模型能较好地跟踪换道轨迹,且稳态行驶下的路径跟踪最大横向误差为8.1%,但在高速极限工况时路径跟踪适应性较差,而L-MPC策略在高速时具有更好的路径跟踪精度及稳定性,其跟踪误差小于4%。展开更多
阐述了CSRH的跟踪指向校准和天线对基线校准的方法。通过利用观测射电星Cassiopeia A或Cygnus A找出流量最大点以校准天线指向,跟踪观测GPS卫星或射电星,并借鉴Korean Solar Radio Burst Locator(KSRBL)系统的8参数校准法校正由天线安...阐述了CSRH的跟踪指向校准和天线对基线校准的方法。通过利用观测射电星Cassiopeia A或Cygnus A找出流量最大点以校准天线指向,跟踪观测GPS卫星或射电星,并借鉴Korean Solar Radio Burst Locator(KSRBL)系统的8参数校准法校正由天线安装引入的误差,校准后误差RMS值可小于22"。在完成上述单天线指向跟踪校准后,应用《Interferometry and Synthesis in Radio Astronomy》阐述的算法可校准天线对基线误差。展开更多
基金financial support from the National Natural Science Foundation of China (51775402 and U1931139)
文摘The Qi Tai Telescope(QTT),which has a 110 m aperture,is planned to be the largest scale steerable tele-scope in the world.Ideally,the telescope’s repeated pointing accuracy error should be less than 2.5 arc seconds(arcsec);thus,the telescope structure must satisfy ultra-high precision requirements.In this pur-suit,the present research envisages a reverse-design method for the track surface to reduce the difficulty of the telescope’s design and manufacture.First,the distribution characteristics of the test data for the track error were verified using the skewness coefficient and kurtosis coefficient methods.According to the distribution characteristics,the azimuth track error was simulated by a two-scale model.The error of the long period and short amplitude was characterized as large-scale and described by a trigonometric function,while the short period and high amplitude error was characterized as small-scale and simulated by a fractal function.Based on the two-scale model,effect of the error on the pointing accuracy was deduced.Subsequently,the relationship between the root mean square(RMS)of the track error and the RMS of the pointing accuracy error of the telescope was deduced.Finally,the allowable RMS value of the track error was derived from the allowable pointing accuracy errors.To validate the effectiveness of the new design method,two typical radio telescopes(the Green Bank Telescope(GBT)and the Large Millimeter Telescope(LMT))were selected as experimental examples.Through comparison,the theoretical calculated values of the pointing accuracy of the telescope were consistent with the measured values,with a maximum error of less than 10%.
文摘针对自主车辆换道轨迹跟踪精度较低等问题进行了研究。提出了基于轨迹预测的多点预瞄权重增益分配的方法。首先,根据车辆与路径的实时横向偏差以及航向角偏差,建立驾驶员转向模型,获得最优方向盘转角;其次,为了提高车辆换道路径跟踪时的稳定性,采用线性模型预测控制(linear model predictive control,L-MPC)策略设计轨迹跟踪控制器。最后,搭建Carsim&Simulink联合仿真模型,针对不同车速设置对比实验进行分析,结果表明基于轨迹预测的驾驶员模型能较好地跟踪换道轨迹,且稳态行驶下的路径跟踪最大横向误差为8.1%,但在高速极限工况时路径跟踪适应性较差,而L-MPC策略在高速时具有更好的路径跟踪精度及稳定性,其跟踪误差小于4%。
文摘阐述了CSRH的跟踪指向校准和天线对基线校准的方法。通过利用观测射电星Cassiopeia A或Cygnus A找出流量最大点以校准天线指向,跟踪观测GPS卫星或射电星,并借鉴Korean Solar Radio Burst Locator(KSRBL)系统的8参数校准法校正由天线安装引入的误差,校准后误差RMS值可小于22"。在完成上述单天线指向跟踪校准后,应用《Interferometry and Synthesis in Radio Astronomy》阐述的算法可校准天线对基线误差。
