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PL
W artykule przedstawiono wyniki integracji chmur punktów pozyskanych z wykorzystaniem naziemnego skanera laserowego oraz smartfona z sensorem LiDAR. Kompletny zbiór danych posłużył do inwentaryzacji ściany obiektu zabytkowego klasztoru Franciszkanów. W 2019 r. na wniosek upoważnionej osoby dokonano pomiarów obiektu ze względu na zaobserwowane odchylenie ściany budynku spowodowane osiadaniem fundamentów budowli i rozpoczęto prace rewitalizacyjne polegające na wzmocnieniu gruntu pod fundamentami kościoła. Przeprowadzono wiele prac mających na celu zatrzymanie osiadania fundamentów, a także dobudowano i uzupełniono brakujące fragmenty ściany, które miały znaczny wpływ na stabilność obiektu. W 2023 r. powtórzono pomiar, wykorzystując naziemny skaner laserowy i smartfon iPhone 12Pro, aby sprawdzić, czy wykonane prace przyniosły pożądany efekt i zahamowały dalsze odchylenia ścian. Kompletny, zintegrowany zbiór danych posłużył również do wizualizacji ściany po zabiegach konserwatorskich.
EN
The article presents the results of the integration of point clouds obtained using a terrestrial laser scanner and a smartphone with a LiDAR sensor. The complete data set was used to inventory the wall of the historic Franciscan Monastery. In 2019, at the request of the parish priest, the building was measured due to the observed deviation of the building walls caused by the subsidence of the foundations of the building and revitalization works began, consisting in strengthening the ground under the foundations of the church. A number of works were carried out to stop the process of settling the foundations of the monastery, and the missing fragments of the wall were added and supplemented, which had a significant impact on the stability of the building. In 2023, the measurement was repeated using terrestrial laser scanner and iPhone 12Pro to check whether the applied works had the desired effect and inhibited further deviations of the walls. A complete, integrated data set was also used to visualize the wall after conservation treatments.
EN
Modern space measurement techniques like SLR, DORIS, VLBI and GNSS are used to study the tectonic plates. The determination of plate motion parameters (Φ, Λ, ω) from various geodetic measurements is outlined. This paper is the third part of our studies on estimating geodetic and geodynamic parameters; it regards an accuracy analysis of the determined Φ, Λ, ω parameters which describe motions of the tectonic plates using Very Long Base Interferometry (VLBI) technique. Prior to this, SLR and DORIS space measurement techniques were examined by authors. The study is based on the velocities of station positions, as included in a realization of the International Terrestrial Reference System - ITRF2008 for VLBI technique, published by the International Earth Rotation and Reference Systems Service (IERS). This model is made subject to an analysis in association with the APKIM2005 model. Six big plates, namely: Eurasian (EUAS), African (AFR), Australian (AUS), North American (NOAM), Pacific (PACF) and Antarctic (ANTC) were analysed. The results obtained in this analysis were compared with our previous estimations based on DORIS and SLR techniques and estimated according to the APKIM2005 model. Generally, all our three solutions based on SLR, DORIS and VLBI measurement techniques were found to be consistent.
EN
One of the primary objectives of satellite geodesy is the determination of coordinates of the satellite laser ranging (SLR) stations. This task is conducted by using laser ranging techniques. The main goal of the current study was to assess the influence of using varied values of the tidal parameters (Love h2 and Shida l2 numbers) on the determination of the positions of chosen SLR stations. The obtained results are presented for coordinates determination conducted for six SLR stations: Mt Stromlo (no. 7825, Australia), Matera (no. 7941, Italy), Grasse (no. 7845, France), McDonald (no. 7080, USA), Arequipa (no. 7403, Peru) and Beijing (no. 7249, China). The analysis covers SLR data for 2 satellites (LAGEOS1 and LAGEOS2), which were observed for 10 consecutive years (from 2008 to 2018). The analysis was performed using the ITRF2014 reference frame in two scenarios of calculations. In scenario 1, the SLR stations coordinates were calculated using the nominal values as per the International Earth Rotation and Reference System Service (IERS) standards recommendation of the Love/Shida numbers: h2 = 0.6078, l2 = 0.0847. In scenario 2, the coordinates were estimated using the harnessing values of the Love/Shida numbers (h2 = 0.6140 and l2 = 0.0876), which were proposed by authors in a previous publication. The effect of the application of different values of the Love/Shida numbers for the determination of SLR stations coordinates was scrutinized.
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