1 / 7

MAGE Mid-term review (23/09/04): network report

MAGE Mid-term review (23/09/04): network report. * Financial support provided through the European Community's Improving Human Potential Program under contract RTN2-2002-00217, MAGE. S. Pireaux. MAGE factual information:. Name: Sophie PIREAUX Nationality: Belgian.

becca
Download Presentation

MAGE Mid-term review (23/09/04): network report

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. MAGE Mid-term review (23/09/04):network report * Financial support provided through the European Community's Improving Human Potential Program under contract RTN2-2002-00217, MAGE S. Pireaux

  2. MAGE factual information: Name: Sophie PIREAUX Nationality: Belgian Age at appointment: 28 Start of appointment: 1st January 2003 End of appointment: 31st December 2004 Category: post-doc Specialty:-relativistic gravitation - IAU recommendations (relativistic ref. systems, space-time transfo, metric) - PPN formalism for testing alternative theories of gravitation - satellites and laser ranging tests of relativity Place of work:UMR5562 Dynamique Terrestre et Planétaire (DTP) Groupe de Recherche en Géodésie Spatiale (GRGS)Observatoire Midi-Pyrénées, Toulouse Country of work:France Previous experience in network: none

  3. Sketches of the young researcher: • A/ Scientific background: • Sept 02-Sept 98: PhD, research assistant, doctoral school, FYMA, UCL (Belgium) • Thesis:“Light deflection experiments as a test of relativistic theories of gravitation.” • Advisor: JM. Gérard • Contract: UCL researcher on exterior funds (IISN, convention n°4.4509.86.051) • 15 Nov 02 – 31 Dec 02: Assistant INSU/CNRS, DTP, OMP (France) • Jan 03 – Dec 04: present MAGE post-doc • B/ Future: • Jan 2005- Dec 2006 (or 2007?):CNES Post-doc, UMR GEMINI, OCA (France) • Subject: ``Solar astrodynamics and relativistic spin-orbit coupling'', • Collaboration: JP. Rozelot, E. Bois • …: apply to CNRS/CNAP, UMR ARTEMIS, OCA • Subject:``Tensor Scalar signatures in gravitational wave emission and detection with LISA?'' • Collaboration: with B. Chauvineau.

  4. Mobility: • contacts with geodesy community: their needs relativistic gravitation? a synergy gravitational theoreticians geodesists is crucial! • contacts with previous institute: regular home missions • Interesting research project: good prospects • native relativistic approach ultimately needed C/ Comments on present post-doctoral position: Advantages: • Drawbacks: • Ambitious project: single person, 2-year post-doc • Presently no joined effort …but GRGS expressed interest at GRGS Summer School 2004 ???

  5. (Semi-Classical) Relativistic Motion Integrator Collaborators: Observatoire Midi-Pyrénées • JP. Barriot • P. Rosenblatt Royal Observatory of Belgium MAGE research subject: « Integrating the motion of satellites in a consistent relativistic framework »

  6. Achievements: basis of RMI software First post-doctoral year: • Study of IAU2000 conventions for astronomy / space-astrometry • Comparison of different relativistic time transfo TT-DTB: SOFA libraries (IAU 2003), DE405 Time-Ephemeris (Irwin and Fukushima, 1999) • Implement transfo between different time scales: TAI , TT, t, TDB, TCB, TCG • Basis of native relativistic software: implementation for simple metrics (Schwarzschild, Kerr, mono / multi-pole) • Started implementation of GCRS metric recommended by the IAU2000 resolutions • Started implementation of new NRO model for Earth rotation (IAU2000) 2nd post-doctoral year • How non-gravitational forces fit in the relativistic framework • How relativistic equations with non-gravitational forces reduce to the classical ones • Order of magnitude of relativistic corrections

  7. Contact Sophie.Pireaux@cnes.fr Projects for the near future: develop RMI software What still needs to be done: • Continue implementation of IAU 2000 GCRS metric • Continue implementation of coordinate transfo • Verify internal / external coherence of ephemeris, astronomical constants used • Make actual comparisons with pre-existing classical orbitography softwares • Symplectic numerical integrator to conserve norm of quadrivector propre velocity • Transpose results to the case of a probe orbiting Mars

More Related