The Compatibility of DORIS with VGOS
| Autor: | Bautista-Duran, Marta, Ferreira, Joao, Garcia, Susana, Hase, Hayo, Kallunki, Juha, Lindqvist, Michael, Madkour, Waleed, Probst, Willi, Tangen, Leif-Morten, Tornatore, Vincenza, Winkel, Benjamin |
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| Rok vydání: | 2023 |
| Předmět: | |
| DOI: | 10.5281/zenodo.8092006 |
| Popis: | In global geodesy co-location of geodetic space techniques are required for mutual control of the measurements. The ground-based active transmitters of the DORIS system are in conflict to VLBI-observations. The VLBI systems are designed to receive extremely faint cosmic signals down to -110 dBm , whereas the DORIS beacon emits signals at a frequency of 2,036 MHz with 40 dBm output power . There is a potential for coupling between DORIS emissions and the VLBI receiving chain generating spurious signals. The selection of possible sites for DORIS next to a VLBI radio telescope have been studied with pycraf. The study results coincide well with real measurements at the site of Wettzell. DORIS can´t be installed in the line of sight with a radio telescope. The complete study is available as living document at https://www.craf.eu/wp-content/uploads/2023/05/DORIS_VGOS_compatibility_study.pdf |
| Databáze: | OpenAIRE |
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