4’th Oersted International Science Team Conference

British Geological Survey, United KingdomBall Aerospace & Technologies Corp., USACarpathian Branch of Subbotin Institute of GeophysicsCentre d'Etude des Environnements Terrestre et PlanétairesCentre Nationale d'Etude Spatiale, FranceDanish Meteorological InstituteDanish Space Research InstituteECMWF, United KingdomESA/ESTEC, HollandFinnish Meteorological InstituteGeoForschungsZentrum Potsdam, GermanyGeological Survey of CanadaGerman Aerospace Center (DLR)Harvard University, USAHermanus Magnetic Observatory, South AfricaIFAC-CNR, ItalyINGV - Geomagnetism, ItalyInst. Atm. Phys., University of Arizona, USAInstitut de Physique du Globe de Paris, France

The Ørsted Satellite

Peter Stauning. Danish Meteorological Institute. February 2004. pst@dmi.dk

4'th Oersted International Science Team ConferenceIDA Conference Centre, Copenhagen, Denmark

Monday 23 - Friday 27, September, 2002

The OIST-4 Conference was arranged jointly by The Danish Meteorological Institute (DMI). The Danish Space Research Institute (DSRI), The Danish Technical University (DTU), and Copenhagen University (CU),

The Ørsted Conference arrangement was sponsored byThe Central Organization of Industrial Employees, Confederation of the Danish Industries, The Society of Danish Engineers, and The Danish Space Research Advisory Board

The OIST-4 Conference had these 6 main themes:  Mapping and modelling of main magnetic field. Includes modelling and interpretation of time varying core field (geo-dynamo), crustal static anomaly fields (Lithosphere), induction fields, and comprehensive modelling of all sources. Mapping and modelling of currents in space. Includes modelling and interpretation of field-aligned currents (FAC) at high, medium and low latitudes, ionospheric currents, ring current, tail and boundary currents. Ionospheric sounding by GPS-based methods. Includes profiling techniques and results, and assimilation of GPS data in regional or global ionospheric models. Atmospheric sounding by GPS-based methods. Includes profiling techniques and results, and assimilation of GPS data in regional or global atmospheric models, numerical weather forecast models and climate models. Advanced instrumentation. Includes state-of-the art techniques for Star Imager, Magnetometer, and Precision GPS Receiver satellite instrumentation. New satellite missions. Includes approved or planned satellite missions with star imager, magnetometer or GPS instrumentation.

Ohio State University, USARaytheon ITSS at GSFC/NASA, USASejong University, KoreaSouthern Illionois University Carbondale, USASPbF IZMIRAN, RussiaTelespazio S.p.A. Earth Obs. Program, ItalyTexas A&M University, USAThe Florida State University, GFDI, USATRW Systems & Information Technology Group, USAUniversity of Bath, United KingdomUniversity of California at San Diego, USAUniversity of Graz, AustriaUniversity of Leipzig, GermanyUniversity of Michigan, USAUniversity of Newcastle, United KingdomUniversity of Sydney, AustraliaU.S. Air Force Research Lab, Hanscom, USAØrsted-DTU, Denmark

Institute of Geodesy and Geophysics; AustriaInstitute of Geophysics and Engineering Seismology, ArmeniaInstitute for Geophysics, Astrophysics and Met., AustriaInstitute of Space and Astronautical Science, JapanIstituto Nazionale di Geofisica e Vulc., ItalyIZMIRAN, RussiaJohns Hopkins University Applied Physics Laboratory, USA JPL/Caltech, USAJPL, NASA, USAKorea Ocean Research and Development InstituteKyoto University, JapanLa Trobe University, AustraliaLeeds University, United KingdomMagnametrics, CanadaMax-Planck Institute für Aeronomie, GermanyMet. Office, United KingdomMission Research Corp., USANASA, Goddard Space Flight Center, USANBI, Copenhagen University

Institutions participating in the 4’th Oersted Insternational Science Team Conference held in Copenhagen

Exhibition ”Ørsted-to-Ørsted held during OIST-4. Right: Ørsteds original compass. Below: Overview of exhibition