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SFB 1128:  Relativistic Geodesy and Gravimetry with Quantum Sensors - Modelling, Geo-Metrology and Future Technology (geo-Q)

Subject Area Geosciences
Computer Science, Systems and Electrical Engineering
Physics
Term from 2014 to 2019
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 239994235
 
Final Report Year 2019

Final Report Abstract

Climate change is one of the greatest challenge of the present time. We are only able to understand the processes relevant for these changes if we analyse the temporal and spatial variations of the gravitational field of the Earth. Gravitational data allow quantifying mass variations such as the mass loss of polar ice sheets, the contribution of mass influx to sea level rise, and changes in the hydrological cycle. Gravitational data are also urgently needed to improve the reference systems used in geodesy and Earth observation. The scientific challenges are threefold: • to determine and monitor global and regional gravity and mass variations from processes that cannot be resolved with the accuracy of current gravitational measurement techniques; • to determine gravity variations with the spatial resolution that is needed for a detailed understanding of mass redistribution and for the separation of sources and mechanisms; • to provide an accurate gravity reference for monitoring processes over long time scales as a basis to reliable quantify both long-term changes and rapid variations. To meet these challenges, new concepts for observing mass variations are required. geo-Q has integrated expertise from geodesy and physics in a unique constellation. geo-Q studied and developed fundamentally new sensors and measurement techniques based on quantum metrology. We investigated laser interferometric systems for ranging between test masses in orbit for satellite gravimetry, with noise levels of nanometers over large distances, and picometers locally, in configurations that allow suitable spatial and temporal sampling of gravity variations. We have succeeded in characterising major noise sources in spaceborne laser interferometry and developed tools to mitigate them. Here, geo-Q crucially benefited from knowledge transfer from the very successful mission “LISA Pathfinder (LPF)” (2015 - 2017) to gravity field missions. The mission GRACE Follow-On (GRACE-FO) (launched in 2018) already profits from this cross-fertilisation. Experiences from geo-Q will be essential to future satellite gravimetry concepts. In geo-Q we also studied and developed atomic gravity sensors for rapid and very precise gravity sensing, based on matter wave interferometry with atoms in the nano-Kelvin to pico-Kelvin temperature regime. These developments enable both compact, mobile devices for field campaigns and large-scale stationary devices for extreme precision. While the former allows for new strategies for local and regional gravity surveys, the latter is able to serve as new gravity standard in the future. geo-Q heralded a paradigm change in atom interferometry, demonstrating a quantum gravimeter employing interferometry with Bose-Einstein condensates created on atom chips. As a third pillar, geo-Q pioneered the concept of relativistic geodesy and addressed its practical application for the realisation of physical height systems and gravity field observations. Key is the observation and comparison of the gravitational frequency redshift over long distances on Earth to determine gravitational potential differences in geodetic networks, using transportable optical atomic clocks and frequency transfer in optical fibre networks. Successful measurements were obtained between Paris and Braunschweig at the 10^−17 level for the relative frequency difference. Along with the research on measurement systems and techniques, where more and more accurate data have been obtained, we also put the analysis models on a sound theoretical basis. This required dedicated relativistic modelling of the various involved gravity field quantities and measurement concepts. A general relativistic definition of the geoid has been developed and it was shown that the resulting “isochronometric surfaces” obtained from clock measurements are mathematically equivalent to a definition based on the levelling approach. In preparation for networks of clocks which can enable stabilisation of height systems, synthetic clock data has been used to identify how many clocks (≥ 4) are required to improve the solution when combined with classical geodetic observables. Furthermore, a framework has been developed to test general relativity through clocks. These clocks and concepts enable new developments for the needs in geodesy, such as unifying height systems and gravity field recovery in the future. Geodetic projects supported the development of novel concepts meeting the requirements on Earth observation and studied the best possible exploitation of these new data. We now know how to deal with disturbing signals in inter-satellite range-rate measurements and are also able to handle potentially disturbing signals affecting clock measurements. geo-Q succeeded in determining a highly accurate static gravity field by combining spaceborne gravimetry and terrestrial data. Our development and realisation of new concepts for observing mass variations in geo-Q enables the acquisition of crucial quantitative input for climate change research with corresponding enormous impact on the whole field of geoscience.

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