space ties
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2021 ◽  
Author(s):  
Grzegorz Bury ◽  
Krzysztof Sośnica ◽  
Radosław Zajdel ◽  
Dariusz Strugarek ◽  
Urs Hugentobler

<p>All satellites of the Galileo and GLONASS navigation systems are equipped with laser retroreflector arrays for Satellite Laser Ranging (SLR). SLR observations to Global Navigation Satellite Systems (GNSS) provide the co-location of two space geodetic techniques onboard navigation satellites.</p><p>SLR observations, which are typically used for the validation of the microwave-GNSS orbits, can now contribute to the determination of the combined SLR+GNSS orbits of the navigation satellites. SLR measurements are especially helpful for periods when the elevation of the Sun above the orbital plane (β angle) is the highest. The quality of Galileo-IOV orbits calculated using combined SLR+GNSS observations improves from 36 to 30 mm for β> 60° as compared to the microwave-only solution. </p><p>Co-location of two space techniques allows for the determination of the linkage between SLR and GNSS techniques in space. Based on the so-called space ties, it is possible to determine the 3D vector between the ground-based co-located SLR and GNSS stations and compare it with the local ties which are determined using the ground measurements. The agreement between local ties derived from co-location in space and ground measurements is at the level of 1 mm in terms of the long-term median values for the co-located station in Zimmerwald, Switzerland.</p><p>We also revise the approach for handling the SLR range biases which constitute one of the main error sources for the SLR measurements. The updated SLR range biases consider now the impact of not only of SLR-to-GNSS observations but also the SLR observations to LAGEOS and the microwave GNSS measurements. The updated SLR range biases improve the agreement between space ties and local ties from 34 mm to 23 mm for the co-located station in Wettzell, Germany.</p><p>Co-location of SLR and GNSS techniques onboard navigation satellites allows for the realization of the terrestrial reference frame in space, onboard Galileo and GLONASS satellites, independently from the ground measurements. It may also deliver independent information on the local tie values with full variance-covariance data for each day with common measurements or can contribute to the control of the ground measurements as long as both GNSS and SLR-to-GNSS observations are available.</p>



2021 ◽  
Author(s):  
Erik Schoenemann ◽  
Florian Dilssner ◽  
Volker Mayer ◽  
Francesco Gini ◽  
Michiel Otten ◽  
...  

<p>The importance of an accurate global geodetic reference frame and associated Earth orientation parameters is undisputed and has been recognised by the UN resolution 69/266. Given the importance of global geodetic references,  ESA is actively contributing to the IAG services: IGS, ILRS, IDS and the contribution to the IVS is in preparation.</p><p>ESA’s activities can be divided into four main areas: the operation of Ground Infrastructure (ESTRACK, EGON, …), the establishment and improvement of inter-technique ties, the operation of a scientific data archive (GSSC) and the generation of geodetic products and services.</p><p>This presentation will focus on the activities performed by the Navigation Support Office. The Navigation Support Office at ESA/ESOC is responsible for providing the Geodetic Reference Frame for all ESA missions and is also the Consortium Coordinator of the Galileo Geodetic Service Provider (GGSP) that generates the Galileo Geodetic Reference Frame (GTRF). Within its responsibilities, the Navigation Support Office is continuously working on improving the consistency of its geodetic products. The possibility to perform a Combination On the Observation Level (CoOL) for all geodetic observations is an excellent tool to identify inconsistencies. Over the recent years, significant improvements have been implemented in the data processing in order to enhance the consistency of the delivered products. As the status of the inter-technique ties remains a limiting factor in this context, ESA is currently investigating the possibility of using space ties, e.g. combining GNSS, SLR, DORIS and VLBI in space.</p><p>This presentation will give an overview of the geodetic products and services generated by ESA’s Navigation Support Office and outline the associated processing setup. In particular, it will report on the analysis performed to improve the consistency of the results provided by the different observation techniques and outline the recent improvements and ongoing activities.</p>



2021 ◽  
Author(s):  
Patrick Schreiner ◽  
Nicat Mammadaliyev ◽  
Susanne Glaser ◽  
Rolf König ◽  
Karl Hans Neumayer ◽  
...  

<p>GGOS-SIM-2, funded by the German Research Foundation (DFG), is a research collaboration project between the German Research Center for Geosciences (GFZ) and the Technische Universität Berlin (TUB). Simulations are utilized to examine the potential of co-location in space, called space ties, of the four main space geodetic techniques, i.e. DORIS, GNSS, SLR and VLBI to achieve the requirements of the Global Geodetic Observing System (GGOS) for a global terrestrial reference frame (TRF), 1 mm accuracy and 1 mm / decade long-term stability. The simulations are performed for six fictional orbit scenarios, including proposed missions GRASP (USA) and E-GRASP (EU), and expanded by a variation of the E-GRASP orbit with lower eccentricity as well as three higher orbiting circular orbits with different inclination over a time span of seven years. For most realistic simulations, we first evaluated real DORIS, GPS and SLR observations to the satellites LAGEOS 1 und 2, Ajisai, LARES, Starlette, Stella, ENVISAT, Jason 1 und 2, Sentinel 3A and B using Precise Orbit Determination (POD), to get detailed information about the individual station and receiver accuracy, availability and further technique-specific effects. Then, we generate simulated single-technique TRF solutions based on existing missions and add the co-location-in-space satellite in the six orbit scenarios. In order to quantify the effects of the different scenarios, we examine the added value w.r.t. the existing missions in terms of origin and scale and of formal errors of the station coordinates and Earth rotation parameters. We also investigate the impact of systematic errors on the derived orbits on the final TRF. The different techniques show individual advantages regarding the respective orbit parameters. For instance, a higher eccentricity of the orbit seems to lead to improved accuracy of length-of-day (LOD) from SLR. The results will help to find the best trade-off for a satellite that co-locates all four techniques in space towards a GGOS-compliant TRF and Earth rotation parameters.</p>



Author(s):  
Nadeshda V. Lukina ◽  

The article is prepared on the base of works by K.F. Karjalainen, A. Kannisto, V.N. Chernetsov, E.I. Rombandeeva, R.K. Bardina, I.N. Gemuev, A.I. Sagalaev, A.V. Baulo. Based on the classification of Karjalainen, the author refers the ancestral (family), village and territorial spirits to the local spirits. By their origin, they are famous ancestors, founders of villages, former personal spirits, and sons of the supreme god Numi-Tōrum. The list of local spirits fixed on the rivers Severnaya Sosva with Ob region, Lyapin / Sygva, Lozva, Pelym, Tavda, Vagilsk, and Konda is given. They are linked to specific loci: villages, forest areas, or water basins. This localization is of two kinds: both the location of the spirit itself and the territory of its worship. These signs do not always coincide. Different variants of the spatial boundaries of worship of a concrete spirit are revealed among the Mansi people. In some cases, only one spirit is worshipped in a village, in other words, it has here "sole" space. In other cases, when different local spirits are worshipped in the same village, their space is common. An even wider area “belongs” to the spirits worshipped in several villages (loci). The most extensive areas of worship were formed by the territorial ancestor spirits. Most of the local spirits were related to each other. This is most clearly demonstrated by the significant territorial spirits whish are considered the children of Numi-Tōrum – Polum-Tōrum, Nyaras-Nāy-Ekva, Tāgt-Kotil-Ōjka, Āj-Ās-Ōjka, and Nyor-Ōjka. In turn, the children of these original patron spirits dispersed to different parts of the Mansi land, becoming the guardians of both the area and the people living in it. These are the nāj-otyrs that helped people to settle where they now live. They are the masters of loci (villages, towns) and are subordinate to one of the most senior original patron spirits. Thus, the sons of Tāgt-Kotil-Ōjka are the patron spirits in several villages on the Severnaya Sosva River, as well as on the Manya River. Seven bogatyr brothers from the Lozva River made military campaigns over the Sosva River. The ties between the nāj-otyrs were often of a warlike nature. They conquered other people's territories and became patron spirits there. The materials presented in the article draw a general picture of the representations about local spirits (ancestral spirits) among different groups of the Mansi people. The basis of these representations is the general Mansi worldview concept about the origin of these characters, about their structure and relationships. The extensive list of ancestral spirits demonstrates, on the one hand, their localization and, on the other hand, the wide spatial area of worship of the most significant of them.



2020 ◽  
Author(s):  
Patrick Schreiner ◽  
Nicat Mammadaliyev ◽  
Susanne Glaser ◽  
Rolf Koenig ◽  
Karl Hans Neumayer ◽  
...  

<p>The German Research Foundation (DFG) project GGOS-SIM-2, successor of project GGOS-SIM, is a collaboration between the Helmholtz Center Potsdam - German Research Center for Geosciences (GFZ) and the Technische Universität Berlin (TUB). The project aims at investigating the feasibility of meeting the requirements specified by the Global Geodetic Observing System (GGOS) for a global terrestrial reference frame (TRF) with the help of simulations. In GGOS-SIM-2 the potential of so-called space ties is examined in relation to the GGOS targets, 1 mm accuracy in position and 1 mm / decade long-term stability, which have not yet been achieved by the recent International Terrestrial Reference Frame (ITRF). Space ties are provided by a satellite that carries two, three or all the four main space-geodetic techniques, i.e. DORIS, GPS, SLR and VLBI. This allows for a quantification of the impact of systematic errors on the derived orbits and subsequent results of the dynamic method as the TRF. Proposed co-location in space missions such as GRASP and E-GRASP anticipate such a scenario. We therefor simulate the space-geodetic observations based on Precise Orbit Determination (POD) with real observations from various missions and evaluate their potential for determining a TRF. So far, we simulated DORIS and SLR observations to six orbit scenarios, including a GRASP-like and an E-GRASP-like one, and generated TRFs based on each scenario either technique-wise or combined via the space-ties or in combination with ground data. We quantify the effect on the TRF in terms of changes of origin and scale and of formal errors of the ground station coordinates and of the Earth rotation parameters.</p>



2020 ◽  
Author(s):  
Michiel Otten ◽  
Tim Springer ◽  
Francesco Gini ◽  
Volker Mayer ◽  
Erik Schoenemann ◽  
...  

<p>For the previous ITRF calls for participation ESOC reprocessed the historic data from the IDS, IGS, and ILRS. Our three solutions were computed with a single software package (NAPEOS), running on the same machine and using, as far as possible, identical settings. Any systematic differences between the technique dependent reference frame solutions must therefore be caused by the techniques themselves, and not because of model differences or errors. Our three technique dependent solutions gave us a good understanding of the technique dependent effects, helping us to improve our models.</p><p>At ESOC we have now made a significant step forward by including all satellite geodetic techniques (SLR, DORIS and GNSS) into one solution. This allows us to combine the ILRS, IDS and IGS reference frames by using “space ties”. Of course these space ties are not perfectly known but they still allow for a rigorous combination of the different reference frames. Furthermore, and very important for the GNSS technique, they allow for the direct estimation of the GNSS satellite transmitter phase centre offset. We solve not only for integer ambiguities of the GPS satellites but also for those of the LEO satellites, which is also providing GPS phase observations on two frequencies. </p><p>Our poster presents an overview of this multi-technique combination approach at observation level (COOL). We have included all observations provided by the following satellites in a single parameter estimation process: GNSS, JASON, SPOT, Sentinels, GRACE, LAGEOS and Etalon satellites. We demonstrate the benefits of such a rigorous approach compared to processing the various space geodetic techniques separately.</p>



2020 ◽  
Author(s):  
Helene Wolf ◽  
Matthias Schartner ◽  
Johannes Böhm ◽  
Andreas Hellerschmied

<p>Observing extragalactic radio sources is an integral part of Very Long Baseline Interferometry (VLBI) but observing satellites also provides a variety of new possibilities. Interesting scientific applications can be found in providing space ties instead of using local ties for connecting reference frames of different space-geodetic techniques. To generate schedules including observations to satellites a dedicated module has been implemented in the new scheduling software VieSched++.</p><p><br>This newly developed module determines possible satellite observations considering several observation conditions, such as the visibility from the selected station network and antenna slew rates. A schedule including observations to quasars and satellites can be generated in a semi-automatic mode. The scheduling of the satellite scans is done manually by the user who can select and adjust the possible satellite observations before adding them to the schedule. The remaining part of the schedule is filled automatically by the software VieSched++ using the general optimization algorithm with observations to quasars. In this poster an overview of the current status of the satellite scheduling module in VieSched++ is given, as well as an outlook to highlight future plans. </p>



2019 ◽  
Vol 93 (11) ◽  
pp. 2379-2387 ◽  
Author(s):  
S. Riepl ◽  
H. Müller ◽  
S. Mähler ◽  
J. Eckl ◽  
T. Klügel ◽  
...  
Keyword(s):  


2017 ◽  
Vol 92 (4) ◽  
pp. 383-399 ◽  
Author(s):  
Sara Bruni ◽  
Paul Rebischung ◽  
Susanna Zerbini ◽  
Zuheir Altamimi ◽  
Maddalena Errico ◽  
...  


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