{"title":"TPL-1望远镜光学通道分离用镜面同步装置","authors":"V. O. Pap, Yu. M. Hlushchenko, M. M. Medvedskiy","doi":"10.3103/S0884591321030065","DOIUrl":null,"url":null,"abstract":"<p>The satellite laser ranging method is based on measuring the transit time of a laser pulse from the transmitter to the satellite and back to the receiver. A special feature of the TPL telescope is that the laser signal is transmitted and received by the same telescope. This requires auxiliary equipment to separate these signals. In addition, this telescope is also used for visual tracking of the object, which adds complexity to the optical design. In most cases, the signals are separated mechanically using rotating mirrors. In one position, the mirrors transmit the signal to a specific channel, and they reflect the optical signal into another channel in the other position. The rotational speed of the mirrors corresponds to the frequency of the laser transmitter. Both mirrors rotate at the same frequency but with a different phase. A logic circuit built on two D-triggers and one 2-input NAND element is used as a phase detector. The paper discusses the scheme and principle of operation of the device for mirror synchronization by signals of the control computer and mirror position sensors. This device has been successfully used at the Riga-1884 laser location station of the University of Latvia.</p>","PeriodicalId":681,"journal":{"name":"Kinematics and Physics of Celestial Bodies","volume":null,"pages":null},"PeriodicalIF":0.5000,"publicationDate":"2021-07-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Mirror Synchronization Unit for Separation of Optical Channels of the TPL-1 Telescope\",\"authors\":\"V. O. Pap, Yu. M. Hlushchenko, M. M. Medvedskiy\",\"doi\":\"10.3103/S0884591321030065\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>The satellite laser ranging method is based on measuring the transit time of a laser pulse from the transmitter to the satellite and back to the receiver. A special feature of the TPL telescope is that the laser signal is transmitted and received by the same telescope. This requires auxiliary equipment to separate these signals. In addition, this telescope is also used for visual tracking of the object, which adds complexity to the optical design. In most cases, the signals are separated mechanically using rotating mirrors. In one position, the mirrors transmit the signal to a specific channel, and they reflect the optical signal into another channel in the other position. The rotational speed of the mirrors corresponds to the frequency of the laser transmitter. Both mirrors rotate at the same frequency but with a different phase. A logic circuit built on two D-triggers and one 2-input NAND element is used as a phase detector. The paper discusses the scheme and principle of operation of the device for mirror synchronization by signals of the control computer and mirror position sensors. This device has been successfully used at the Riga-1884 laser location station of the University of Latvia.</p>\",\"PeriodicalId\":681,\"journal\":{\"name\":\"Kinematics and Physics of Celestial Bodies\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.5000,\"publicationDate\":\"2021-07-02\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Kinematics and Physics of Celestial Bodies\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.3103/S0884591321030065\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Kinematics and Physics of Celestial Bodies","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.3103/S0884591321030065","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
Mirror Synchronization Unit for Separation of Optical Channels of the TPL-1 Telescope
The satellite laser ranging method is based on measuring the transit time of a laser pulse from the transmitter to the satellite and back to the receiver. A special feature of the TPL telescope is that the laser signal is transmitted and received by the same telescope. This requires auxiliary equipment to separate these signals. In addition, this telescope is also used for visual tracking of the object, which adds complexity to the optical design. In most cases, the signals are separated mechanically using rotating mirrors. In one position, the mirrors transmit the signal to a specific channel, and they reflect the optical signal into another channel in the other position. The rotational speed of the mirrors corresponds to the frequency of the laser transmitter. Both mirrors rotate at the same frequency but with a different phase. A logic circuit built on two D-triggers and one 2-input NAND element is used as a phase detector. The paper discusses the scheme and principle of operation of the device for mirror synchronization by signals of the control computer and mirror position sensors. This device has been successfully used at the Riga-1884 laser location station of the University of Latvia.
期刊介绍:
Kinematics and Physics of Celestial Bodies is an international peer reviewed journal that publishes original regular and review papers on positional and theoretical astronomy, Earth’s rotation and geodynamics, dynamics and physics of bodies of the Solar System, solar physics, physics of stars and interstellar medium, structure and dynamics of the Galaxy, extragalactic astronomy, atmospheric optics and astronomical climate, instruments and devices, and mathematical processing of astronomical information. The journal welcomes manuscripts from all countries in the English or Russian language.