European GEOS Mission: the Satellites Geos was designed for geostationary orbit to study the particles, fields and plasmas of the Earth's magnetosphere using seven instruments provided by ten European laboratories. Because of its unique orbit and the sophistication of its payload, Geos was selected as the reference spacecraft for the worldwide 'International Magnetospheric Study'. Unfortunately, Geos-1 was left in a low transfer orbit following launch on 20 April 1977 because of a problem with its US Delta launcher. As a result, the Qualification Model was launched as Geos-2 on 14 July 1978 with an identical payload and successfully reached the planned orbit. In spite of its orbit, Geos-1 made a significant contribution to IMS, and its mission formally ended on 23 June. Geos-2 was highly successful, creating a huge database for magnetospheric studies and plasma research in general. Science objectives of the European GEOS Mission - to advance our knowledge of the dynamics of the magnetosphere, in particular to study the response of the near-Earth environnment to varying conditions in interplanetary space (nominal objective reached with GEOS-2), -to study of the dayside sector of the magnetosphere : the plasma bulge and the plasmapause have been investigated in detail.(GEOS-1). GEOS comprises the following seven experiments: S-300 AC-magnetic fields up to 30 kHz DC/AC electric fields and plasma resonances up to 80 kHz Mutual and self-impedance CRPE, Issy-les-Moulineuax, France Space Science Dept., ESA, ESTAC, Holland Danish Space Research Institute, Lyngby, Denmark CRPE, Orléans, France S-302 Thermal plasma up to 500 eV Mullard Space Science Lab., Dorking, UK S-303 Composition (1-140 amu) and energy spectra of ions up to 16 keV University of Bern, Switzerland Max-Planck-Institut, Garching, Germany S-310 Pitch-angle distribution of electrons and protons (0.2-20 keV) energy range Kiruna Geophysical Observatory, Kiruna, Sweden S-321 Pitch-angle distribution for electrons (20-300 keV) and protons (20 keV-3MeV) Max-Planck-Institut, Lindau, Germany S-329 DC electric field Max-Planck-Institut, Garching, Germany S-331 DC and ULF magnetif field CNR, Frascaty, Italy NASA/GSFC, Greenbelt, Maryland
Version:2.4.0
European GEOS Mission: the Satellites Geos was designed for geostationary orbit to study the particles, fields and plasmas of the Earth's magnetosphere using seven instruments provided by ten European laboratories. Because of its unique orbit and the sophistication of its payload, Geos was selected as the reference spacecraft for the worldwide 'International Magnetospheric Study'. Unfortunately, Geos-1 was left in a low transfer orbit following launch on 20 April 1977 because of a problem with its US Delta launcher. As a result, the Qualification Model was launched as Geos-2 on 14 July 1978 with an identical payload and successfully reached the planned orbit. In spite of its orbit, Geos-1 made a significant contribution to IMS, and its mission formally ended on 23 June. Geos-2 was highly successful, creating a huge database for magnetospheric studies and plasma research in general. Science objectives of the European GEOS Mission - to advance our knowledge of the dynamics of the magnetosphere, in particular to study the response of the near-Earth environnment to varying conditions in interplanetary space (nominal objective reached with GEOS-2), -to study of the dayside sector of the magnetosphere : the plasma bulge and the plasmapause have been investigated in detail.(GEOS-1). GEOS comprises the following seven experiments: S-300 AC-magnetic fields up to 30 kHz DC/AC electric fields and plasma resonances up to 80 kHz Mutual and self-impedance CRPE, Issy-les-Moulineuax, France Space Science Dept., ESA, ESTAC, Holland Danish Space Research Institute, Lyngby, Denmark CRPE, Orléans, France S-302 Thermal plasma up to 500 eV Mullard Space Science Lab., Dorking, UK S-303 Composition (1-140 amu) and energy spectra of ions up to 16 keV University of Bern, Switzerland Max-Planck-Institut, Garching, Germany S-310 Pitch-angle distribution of electrons and protons (0.2-20 keV) energy range Kiruna Geophysical Observatory, Kiruna, Sweden S-321 Pitch-angle distribution for electrons (20-300 keV) and protons (20 keV-3MeV) Max-Planck-Institut, Lindau, Germany S-329 DC electric field Max-Planck-Institut, Garching, Germany S-331 DC and ULF magnetif field CNR, Frascaty, Italy NASA/GSFC, Greenbelt, Maryland
Role | Person | |
---|---|---|
1. | ProjectScientist | spase://CNES/Person/CDPP-Archive/Karl.Knott |