克里米亚地球动力试验区台站网络:局部联系变化及其与ITRF2020参考框架中获得的值的比较

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Kinematics and Physics of Celestial Bodies Pub Date : 2023-05-24 DOI:10.3103/S0884591323020046
O. Khoda, Ya. Yatskiv
{"title":"克里米亚地球动力试验区台站网络:局部联系变化及其与ITRF2020参考框架中获得的值的比较","authors":"O. Khoda,&nbsp;Ya. Yatskiv","doi":"10.3103/S0884591323020046","DOIUrl":null,"url":null,"abstract":"<p>The Simeiz–Katzively Crimean geodynamic test area is one of the unique site in the world, in which several space geodesy observation stations are located, namely, RT-22 radio telescope (CRIMEA, CDP no. 7332), satellite laser ranging (SLR) stations 1873 Simeiz and 1893 Katzively, permanent GNSS stations CRAO and KTVL, and the marker of mobile SLR station 7561 Simeiz. Four local survey geodetic campaigns and five GNSS campaigns were performed to determine local ties between space geodesy stations and basic markers on this site. As a result of campaigns, the coordinates of points (space geodesy stations and markers) in the Simeiz–Katzively Crimean geodynamic test area in the ITRF2000 reference frame at epoch 2004.6 were estimated. Local ties between basic site points were determined as differences between positions of the corresponding points and the position of the RT-22 radio telescope. Deviations from the average values of local ties at the sites of the RT-22 radio telescope and the SLR station of CrAO vary within the limits of up to 3.6 and 6.4 mm, respectively. Actually, they are within the limits of determination errors of local ties. The wide range of local ties variations for the mobile SLR station (7561) is caused by the physical damage of this marker and excavation works carried out around it between observation campaigns. The local ties for points at the site of the SLR station of CLO of the Main Astronomical Observatory of the National Academy of Sciences of Ukraine vary in a very wide range because this site has a local movement in the southern direction with a substantial velocity. The coordinates of the space geodesy stations in the Simeiz–Katzively Crimean geodynamic test area are available in the ITRF2020 catalogue, so it was possible to compare the local ties calculated from its data with the ones obtained by processing the data of geodetic campaigns. The differences between the two types of local ties are very large (up to 45 mm). The reasons for these discrepancies could lie both in the errors of local ties obtained during the geodetic campaigns and in the errors of estimates of the space geodesy station coordinates at this site in the ITRF2020 catalog. The distance between SLR station 1893 Katzively and the RT-22 radio telescope (1893–7332) shows a special behavior due to the fact that the velocities given in the ITRF2020 catalog for all SLR stations at the Simeiz–Katzively Crimean geodynamic test area have the same values and, consequently, substantial local movements of the site around the 1893 Katzively station are not taken into account. Considering the substantial local movements of this site, the velocities of SLR stations at the Simeiz–Katzively Crimean geodynamic test area should be estimated separately for each station for future implementations of the International Terrestrial Reference System (ITRS), as has been done, for example, for permanent GNSS stations CRAO and KTVL.</p>","PeriodicalId":681,"journal":{"name":"Kinematics and Physics of Celestial Bodies","volume":"39 2","pages":"116 - 122"},"PeriodicalIF":0.5000,"publicationDate":"2023-05-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Network of Stations of the Crimean Geodynamic Test Area: Local Ties Variations and Their Comparison with the Values Obtained in the ITRF2020 Reference Frame\",\"authors\":\"O. Khoda,&nbsp;Ya. Yatskiv\",\"doi\":\"10.3103/S0884591323020046\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>The Simeiz–Katzively Crimean geodynamic test area is one of the unique site in the world, in which several space geodesy observation stations are located, namely, RT-22 radio telescope (CRIMEA, CDP no. 7332), satellite laser ranging (SLR) stations 1873 Simeiz and 1893 Katzively, permanent GNSS stations CRAO and KTVL, and the marker of mobile SLR station 7561 Simeiz. Four local survey geodetic campaigns and five GNSS campaigns were performed to determine local ties between space geodesy stations and basic markers on this site. As a result of campaigns, the coordinates of points (space geodesy stations and markers) in the Simeiz–Katzively Crimean geodynamic test area in the ITRF2000 reference frame at epoch 2004.6 were estimated. Local ties between basic site points were determined as differences between positions of the corresponding points and the position of the RT-22 radio telescope. Deviations from the average values of local ties at the sites of the RT-22 radio telescope and the SLR station of CrAO vary within the limits of up to 3.6 and 6.4 mm, respectively. Actually, they are within the limits of determination errors of local ties. The wide range of local ties variations for the mobile SLR station (7561) is caused by the physical damage of this marker and excavation works carried out around it between observation campaigns. The local ties for points at the site of the SLR station of CLO of the Main Astronomical Observatory of the National Academy of Sciences of Ukraine vary in a very wide range because this site has a local movement in the southern direction with a substantial velocity. The coordinates of the space geodesy stations in the Simeiz–Katzively Crimean geodynamic test area are available in the ITRF2020 catalogue, so it was possible to compare the local ties calculated from its data with the ones obtained by processing the data of geodetic campaigns. The differences between the two types of local ties are very large (up to 45 mm). The reasons for these discrepancies could lie both in the errors of local ties obtained during the geodetic campaigns and in the errors of estimates of the space geodesy station coordinates at this site in the ITRF2020 catalog. The distance between SLR station 1893 Katzively and the RT-22 radio telescope (1893–7332) shows a special behavior due to the fact that the velocities given in the ITRF2020 catalog for all SLR stations at the Simeiz–Katzively Crimean geodynamic test area have the same values and, consequently, substantial local movements of the site around the 1893 Katzively station are not taken into account. Considering the substantial local movements of this site, the velocities of SLR stations at the Simeiz–Katzively Crimean geodynamic test area should be estimated separately for each station for future implementations of the International Terrestrial Reference System (ITRS), as has been done, for example, for permanent GNSS stations CRAO and KTVL.</p>\",\"PeriodicalId\":681,\"journal\":{\"name\":\"Kinematics and Physics of Celestial Bodies\",\"volume\":\"39 2\",\"pages\":\"116 - 122\"},\"PeriodicalIF\":0.5000,\"publicationDate\":\"2023-05-24\",\"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/S0884591323020046\",\"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/S0884591323020046","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}
引用次数: 0

摘要

simez - katzively克里米亚地球动力学试验区是世界上独一无二的试验区之一,其中有几个空间大地测量观测站,即RT-22射电望远镜(克里米亚,CDP号)。7332),卫星激光测距站1873 simez和1893 Katzively,永久GNSS站CRAO和KTVL,以及移动SLR站7561 simez的标记。进行了四次地方大地测量运动和五次GNSS运动,以确定该站点空间大地测量站与基本标记之间的地方联系。作为这些运动的结果,在ITRF2000参考框架中估计了2004.6历元时Simeiz-Katzively克里米亚地球动力学试验区的点坐标(空间大地测量站和标记)。基本站点点之间的局部联系被确定为对应点的位置与RT-22射电望远镜位置之间的差异。RT-22射电望远镜和cro单反站的局地连线平均值与局地连线平均值的偏差分别在3.6 mm和6.4 mm以内。实际上,它们都在局部关系的判定误差范围内。移动单反站(7561)的地方联系差异很大,这是由于该标记的物理损坏以及在观测活动之间在其周围进行的挖掘工作造成的。乌克兰国家科学院主天文台CLO单反站站点各点的地方联系变化很大,因为该站点有一个向南方向的速度很大的局部运动。ITRF2020目录中提供了Simeiz-Katzively Crimean地球动力学试验区空间大地测量站的坐标,因此可以将其数据计算的局部联系与处理大地测量运动数据获得的当地联系进行比较。两种局部扎带之间的差异非常大(最大可达45mm)。造成这些差异的原因可能是在大地测量运动期间获得的当地联系的错误,以及ITRF2020目录中对该场址空间大地测量站坐标的估计的错误。1893 Katzively SLR站与RT-22射电望远镜(1893 - 7332)之间的距离表现出一种特殊的行为,这是由于ITRF2020目录中给出的simez - Katzively克里米亚地球动力学试验区所有SLR站的速度值相同,因此没有考虑1893 Katzively站周围站点的大量局部运动。考虑到该场址的大量局部运动,为今后实施国际地面参考系统(ITRS), Simeiz-Katzively Crimean地球动力学试验区的SLR站的速度应分别为每个站进行估计,例如为GNSS永久站CRAO和KTVL所做的工作。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

摘要图片

查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
Network of Stations of the Crimean Geodynamic Test Area: Local Ties Variations and Their Comparison with the Values Obtained in the ITRF2020 Reference Frame

The Simeiz–Katzively Crimean geodynamic test area is one of the unique site in the world, in which several space geodesy observation stations are located, namely, RT-22 radio telescope (CRIMEA, CDP no. 7332), satellite laser ranging (SLR) stations 1873 Simeiz and 1893 Katzively, permanent GNSS stations CRAO and KTVL, and the marker of mobile SLR station 7561 Simeiz. Four local survey geodetic campaigns and five GNSS campaigns were performed to determine local ties between space geodesy stations and basic markers on this site. As a result of campaigns, the coordinates of points (space geodesy stations and markers) in the Simeiz–Katzively Crimean geodynamic test area in the ITRF2000 reference frame at epoch 2004.6 were estimated. Local ties between basic site points were determined as differences between positions of the corresponding points and the position of the RT-22 radio telescope. Deviations from the average values of local ties at the sites of the RT-22 radio telescope and the SLR station of CrAO vary within the limits of up to 3.6 and 6.4 mm, respectively. Actually, they are within the limits of determination errors of local ties. The wide range of local ties variations for the mobile SLR station (7561) is caused by the physical damage of this marker and excavation works carried out around it between observation campaigns. The local ties for points at the site of the SLR station of CLO of the Main Astronomical Observatory of the National Academy of Sciences of Ukraine vary in a very wide range because this site has a local movement in the southern direction with a substantial velocity. The coordinates of the space geodesy stations in the Simeiz–Katzively Crimean geodynamic test area are available in the ITRF2020 catalogue, so it was possible to compare the local ties calculated from its data with the ones obtained by processing the data of geodetic campaigns. The differences between the two types of local ties are very large (up to 45 mm). The reasons for these discrepancies could lie both in the errors of local ties obtained during the geodetic campaigns and in the errors of estimates of the space geodesy station coordinates at this site in the ITRF2020 catalog. The distance between SLR station 1893 Katzively and the RT-22 radio telescope (1893–7332) shows a special behavior due to the fact that the velocities given in the ITRF2020 catalog for all SLR stations at the Simeiz–Katzively Crimean geodynamic test area have the same values and, consequently, substantial local movements of the site around the 1893 Katzively station are not taken into account. Considering the substantial local movements of this site, the velocities of SLR stations at the Simeiz–Katzively Crimean geodynamic test area should be estimated separately for each station for future implementations of the International Terrestrial Reference System (ITRS), as has been done, for example, for permanent GNSS stations CRAO and KTVL.

求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
Kinematics and Physics of Celestial Bodies
Kinematics and Physics of Celestial Bodies ASTRONOMY & ASTROPHYSICS-
CiteScore
0.90
自引率
40.00%
发文量
24
审稿时长
>12 weeks
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.
期刊最新文献
Estimation of Velocities of Ukrainian GNSS Stations in the IGb08 Reference Frame A Study of Dynamics of Changes in Parameters of the Chandler Pole Oscillation in the Period 1975.0–2011.0 A Spectral Study of Active Region Site with an Ellerman Bomb and Hα Ejections: Chromosphere. Arch Filament System Plane Internal Gravity Waves with Arbitrary Amplitude A Statistical Study of the CME Properties Based on Angular Width during the Solar Cycle 24
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1