G53A:
Relativistic Geodesy and Quantum Sensors for Geodesy II

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Session ID#: 16011

Session Description:
Relativistic geodesy finds very strong interest today. It is a field where fundamental progress in metrology and sensors – including quantum metrology and quantum sensors – together with modeling advances enable new and very relevant applications. Optical atomic clocks achieve relative frequency accuracies in the 10-18 range, and long-distance frequency transfer has even been demonstrated with 10-19 accuracy. These techniques open the perspective for tying potential and height differences to an atomic reference, possibly in global geodetic networks. Quantum inertial sensors based on atom interferometry are very promising with respect to compactness, accuracy and versatility for geodetic applications on ground and in space. Complementarily, the space missions LISA Pathfinder, Microscope and GRACE Follow-On are achieving major advances in precision ranging and accelerometry. The session provides a forum for exchange on theory, sensors and applications for gravity field determination and navigation.
Primary Convener:  Jakob Flury, Leibniz University of Hannover, Hannover, Germany
Conveners:  Jun Ye, JILA, NIST and University of Colorado, Boulder, CO, United States, Mark Kasevich, Stanford University, Stanford, CA, United States and Pacôme Delva, SYRTE, Observatoire de Paris, Paris, France
Chairs:  Jakob Flury, Leibniz University of Hannover, Hannover, Germany and Pacôme Delva, SYRTE, Observatoire de Paris, Paris, France
OSPA Liaison:  Pacôme Delva, SYRTE, Observatoire de Paris, Paris, France
Index Terms:

1214 Geopotential theory and determination [GEODESY AND GRAVITY]
1229 Reference systems [GEODESY AND GRAVITY]
1244 Standards and absolute measurements [GEODESY AND GRAVITY]
1294 Instruments and techniques [GEODESY AND GRAVITY]

Abstracts Submitted to this Session:

Christian Lisdat, Silvio B. Koller, Jacopo Grotti, Stefan Vogt, Ali Al-Masoudi, Sören Dörscher, Sofia Herbers, Sebastian Häfner and Uwe Sterr, PTB Physikalisch-Technische Bundesanstalt, Braunschweig, Germany
Juergen Mueller, Leibniz University of Hannover, Institut für Erdmessung, Hannover, Germany and Jakob Flury, Leibniz University of Hannover, Hannover, Germany
Pacôme Delva, Neus Puchades and Jérôme Lodewyck, LNE–SYRTE, Observatoire de Paris, CNRS (UMR8630), UPMC, SYRTE, Paris, France
Sergei M Kopeikin1,2, Alexander P. Karpik2, Alexander S. Tolstikov3, Elena G. Gienko2, Irina G. Ganagina2 and Elena M. Mazurova2,4, (1)University of Missouri, Department of Physics & Astronomy, Columbia, MO, United States, (2)Siberian State University of Geosystems and Technologies, Physical Geodesy and Remote Sensing, Novosibirsk, Russia, (3)Siberian Science Research Institute of Metrology, Time Metrology and Earth Rotation, Novosibirsk, Russia, (4)MIIGAiK, Department of Geodesy, Moscow, Russia
Geoffrey Blewitt1,2, Benjamin M Roberts1, Conner Dailey1, Maxim Pospelov3,4, Alex Rollings1, Jeff Shermann5, Wyatt Williams1 and Andrei Derevianko1, (1)University of Nevada, Department of Physics, Reno, NV, United States, (2)University of Nevada, Nevada Geodetic Laboratory, Nevada Bureau of Mines & Geology, Reno, NV, United States, (3)University of Victoria, Department of Physics and Astronomy, Victoria, BC, Canada, (4)Perimeter Institute for Theoretical Physics, Waterloo, ON, Canada, (5)National Institute of Standards and Technology Boulder Laboratories, Boulder, CO, United States
Scott B Luthcke1, Babak Saif2, Alex Sugarbaker3, David D Rowlands2 and Bryant D Loomis4, (1)NASA Goddard Space Flight Center, Greenbelt, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)AOSense Inc., Sunnyvale, CA, United States, (4)Stinger Ghaffarian Technologies (SGT), Greenbelt, MD, United States
Olivier Carraz1, Massotti Luca1, Christian Siemes2, Roger Haagmans3 and Pierluigi Silvestrin1, (1)European Space Agency, Villanueva De La Can, Spain, (2)RHEA System, Wavre, Belgium, (3)ESTEC, Noordwijk, Netherlands

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