A novel Doppler frequency measurement method based on the closed-loop signal correlation for deep sp

来源 :天文和天体物理学研究 | 被引量 : 0次 | 上传用户:godmouse
下载到本地 , 更方便阅读
声明 : 本文档内容版权归属内容提供方 , 如果您对本文有版权争议 , 可与客服联系进行内容授权或下架
论文部分内容阅读
In deep space exploration,it is necessary to improve the accuracy of frequency measurement to meet the requirements of precise orbit determination and various scientific studies.A phase detector is one of the key modules that restricts the tracking performance of phase-locked loop (PLL).Based on the phase relationship between adjacent signals in the time domain,a novel phase detector is presented to replace the arctangent phase detector.The new PLL,which is a closed loop signal correlation algorithm,shows good performance in tracking signals with high precision and the tracking accuracy of frequency of 1 second integration is close to Cramer-Rao lower bound (CRLB) when setting proper parameters.Actual data processing results further illustrate the excellent performance of the novel PLL.
其他文献
In this paper,we present the analysis of the stellar system HIP 101227 to determine the actual number of components in the system,and their properties.We use dynamical modeling and complex spectrophotometric (involving atmospheric modeling) techniques wit
In the past few years,Chinese astronomical community is actively testing astronomical sites for several new optical/infrared ground-based telescopes.These site testing campaigns conducted were mainly focused on fundamental performances of the sites,such a
I find that a (~) 0.1-1 M☉ outflowing equatorial dusty disk (torus) that the binary system progenitor of an intermediate luminosity optical transient (ILOT) ejects several years to several months before and during the outburst can reduce the total emissio
Estimating ages for a large number of giants is of great importance for studying Galactic evolution.In this work,we determine stellar ages and masses for 556007 giants from LAMOST Data Release 5 (DR5)with empirical relations estimated from chemical[C/N]ab
The continuous observation of the magnetic field by the Solar Dynamics Observatory(SDO)/Helioseismic and Magnetic Imager (HMI) produces numerous image sequences in time and space.These sequences provide data support for predicting the evolution of photosp
Data release 2 (DR2) from the Gaia mission was of great help in precise determination of fundamental parameters of Close Visual Binary and Multiple Systems (CVBMSs),especially masses of their components,which are crucial parameters in understanding format
CME is one of the important events in the sun-earth system as it can induce geomagnetic disturbance and an associated space environment effect.It is of special significance to predict whether CME will reach the Earth and when it will arrive.In this paper,
Quasars with periodic light curves are considered as candidates of supermassive binary black hole(BBH) systems.One way for further confirmations may be searching for other characteristic signatures,such as those in their broad emission lines (BELs),if any
The discovery of massive galaxies at high redshifts,especially the passive ones,poses a big challenge for the current standard galaxy formation models.Here we use the semi-analytic galaxy formation model developed by Henriques et al.to explore the formati
In deep space exploration,many engineering and scientific requirements require the accuracy of the measured Doppler frequency to be as high as possible.In our paper,we analyze the possible frequency measurement points of the third-order phase-locked loop