G11A:
Earth and Planetary Rotation: Improving Theories, Models, and Observations I Posters


Session ID#: 10692

Session Description:
Variations in the rotation, precession, and nutation of the Earth and other planets are caused by processes both external and internal to them. For the Earth, the increasing accuracy and temporal resolution of the observations provided by current and next generation measurement systems allow smaller amplitude and higher frequency signals to be observed, motivating improvements in both theories and models of Earth rotation variations. For the other planets, new missions to them will allow better understanding of their rotational variations. These improved theories, models, and observations allow greater understanding of the many processes that are causing the rotation, precession, and nutation of the Earth and other planets to change. This session will be a forum for discussing the improved theories, models, and observations of variations in Earth and planetary rotation.
Primary Convener:  Richard S Gross, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
Conveners:  Aleksander Brzezinski, Warsaw University of Technology, Warszawa, Poland, Veronique M A Dehant, Royal Observatory of Belgium, Brussels, Belgium and Jose M. Ferrandiz, University of Alicante, UAVAC, Applied Mathematics Dept., Alicante, Spain
Chairs:  Richard S Gross, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States and Veronique M A Dehant, Royal Observatory of Belgium, Brussels, Belgium
OSPA Liaison:  Richard S Gross, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States

Cross-Listed:
  • P - Planetary Sciences
Index Terms:

1239 Earth rotation variations [GEODESY AND GRAVITY]
5450 Orbital and rotational dynamics [PLANETARY SCIENCES: SOLID SURFACE PLANETS]
5744 Orbital and rotational dynamics [PLANETARY SCIENCES: FLUID PLANETS]

Abstracts Submitted to this Session:

Veronique M A Dehant, Royal Observatory of Belgium, Brussels, Belgium
Jan M. Hagedoorn, Technical University Berlin, Berlin, Germany, Harald Schuh, Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences, Potsdam, Germany, Matthias Madzak, Federal Office of Metrology and Surveying, Department for Control Survey, Vienna, Austria and Wolfgang Bosch, freelancer, Wolfrathshausen, Germany
Christian Bizouard, Paris Observatory, Paris, France and Christian Bizouard, SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, LNE, Paris, France
Olivier de Viron, U. La Rochelle, LIENSs, La Rochelle, France, Michel J. Van Camp, Observatoire Royal de Belgique, Brussel, Belgium, Paul Rebischung, Université de Paris, Institut de physique du globe de Paris, CNRS, IGN, F-75005 Paris, France and Christian Bizouard, SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, LNE, Paris, France
Richard S Gross, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
KookHyoun Youm1, Taehwan Jeon2, Sung-Ho Na3 and Ki-Weon Seo2, (1)Seoul National University, Seoul, South Korea, (2)Seoul National University, Seoul, Korea, Republic of (South), (3)Ajou University, Suwon, Korea, Republic of (South)
Nicholas G Stamatakos, US Naval Observatory, Washington, DC, United States, Dennis D McCarthy, Retired, Washington, DC, United States, Thomas Marshall Eubanks, Asteroid Initiatives LLC, Virginia, United States and David Salstein, Atmospheric and Environmental Research, Lexington, MA, United States
Leonid Petrov, ADNET Systems @ Geodesy and Geophysics Lab, GSFC, Greenbelt, MD, United States and Christian Bizouard, SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, LNE, Paris, France

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