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Projekt Druckansicht

Investigation of sub-daily and episodic variations of Earth rotation observed by VLBI, ring laser gyroscopes and GNSS

Mitantragsteller Professor Dr. Robert Weber
Fachliche Zuordnung Geophysik und Geodäsie
Förderung Förderung von 2006 bis 2014
Projektkennung Deutsche Forschungsgemeinschaft (DFG) - Projektnummer 5471782
 
Erstellungsjahr 2015

Zusammenfassung der Projektergebnisse

The goal of the project SPEED was to improve our understanding of the high frequency and episodic variations in the rotation of the Earth. In order to investigate these effects we first needed to obtain accurate time series of the Earth rotation parameters (ERP) with high temporal resolution. We estimated the ERP from the space geodetic techniques VLBI and GNSS, as well as observations from ring laser gyroscopes. A lot of progress has been made towards finding the best analysis strategies for the different techniques. For example, we have investigated the effects of radio source position errors in VLBI. We have also developed methods for combining the different ERP time series. Here, one highlight was the successful combination of VLBI and ring laser data at the normal equation level. The benefit of such a combination is currently limited since only one ring laser with high enough accuracy exists, the “G” ring laser in Wettzell. However, simulations have shown that if data of a global network of ring lasers were available there would be a significant improvement in the accuracy compared to the ERP estimated from VLBI data only. Thus ring lasers have the potential to become an important technique for measuring Earth rotation in the future. Kalman filters for combination of hourly ERP for different techniques at the results level were also developed. These Kalman filters were successfully tested by combining ERP from GNSS and VLBI during the continuous VLBI campaigns of the years 2002, 2005, 2008, and 2011. The high frequency ERP time series were applied for estimation of sub-diurnal tidal ERP models. Models derived from GNSS data were compared with models derived from VLBI data. It was found that it is difficult to estimate the tidal coefficients from GNSS data at certain frequencies due to the difficulty to separate the effects of Earth rotation and the effects of the satellite orbits on the GNSS observations. Combined tidal models based on both GNSS and VLBI data were also calculated. The resulting tidal coefficients were compared to those predicted by ocean tide models and libration, i.e. the IERS sub-diurnal ERP model. We concluded that the IERS model contains significant errors – probably because it is based on an old ocean tide model – and it needs to be updated. We have also studied the different geophysical causes for sub-diurnal ERP variations. In particular we have looked at the excitations caused by the atmosphere. Atmospheric angular momentum estimated from different numerical weather models have been investigated and compared to the observed ERP excitations. Another focus was placed on the excitation of Earth rotation caused by earthquakes. Careful modelling of the excitations caused by earthquakes have been made. We have found that the earthquakes of the last 35 years should have changed the mean position of the pole by about 10 mas towards 120°E and shortened the length of day by about 10 μs. Most of this effect are caused by the largest earthquakes (magnitude >8.5). We have tried to detect these changes in the ERP measurements, however, the effect of one single Earthquake is too small compared to the accuracies of the measurements and the modelling of other geophysical excitations of Earth rotation.

Projektbezogene Publikationen (Auswahl)

 
 

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