{
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    "Observatory": {
      "ResourceID": "spase://CNES/Observatory/CDPP-Archive/Interball-Tail",
      "ResourceHeader": {
        "ResourceName": "Interball-Tail",
        "ReleaseDate": "2022-04-28T17:46:51Z",
        "Description": "The TAIL PROBE with its subsatellite was launched on 3 August 1995 to the elongated elliptical orbit with the inclination of 65 degrees and apogee of 200 000 km. These satellites study the interactions of the Solar Wind with the Magnetopause and the outer regions of the magnetosphere. Specific aims is to study the active plasma processes within the tail where powerful currents, substorms and other large-scale non-linear magnetospheric phenomena originate. The separation in this pair will change from less than 100 km, allowing to study the small-scale wave and plasma structures at the boundaries, till about 1-2 RE (the Earth's radii) to study large plasma structures in the tail. \n\nInterball Tail Probe : On-board Experiments\n\nPLASMA\n\nSKA-1\na) Measurements of three-dimensional distribution of ions in the energy range 50 ÷ 5000 eV/Q\nb) Measurements of energy spectra of ions with M/Q selection (M = 1, 2, 4, 16) in the energy range 5-40 ke V/Q in the antisolar direction\nO.VAISBERG, A.LEIBOV, L.AVANOV, IKI Moscow Russia\n\nELECTRON\n3-D measurements of the electron component of the plasma (10 eV - 26 keV)\nJ.A.SAUVAUD, CESR Toulouse France  - O.VAISBERG, N.BORODKOVA, IKI Moscow, Russia\n\nPROMICS-3\nIon composition (M = 1-32) and 3-D energy distribution (0.01-30 ke V/Q)\nI.SANDAHL, IRF, Kiruna, Sweden - N.PISSARENKO, E.DUBININ IKI, Moscow, Russia - H.KOSKINEN, T.PULKKINEN, FMI Helsinki, Finland\n\nVDP\nOmnidirectional fast measurements of integral ion or electron fluxes and their direction\nYa.SAFRANKOVA, Z.NEMECEK Charles Univ., Prague Czech. Republic - G.ZASTENKER, A.FEDOROV IKI, Moscow, Russia\n\nAMEI-2\nEnergy spectra of H+, He+, He++ O+ and heavier ion in the range 0.1-8 ke V/Q at all directions.\nR.KOLEVA STIL, Sofia, Bulgaria - V.SMIRNOV IKI, Moscow, Russia\n\nMONITOR-3\nMeasurements of the solar wind ion fluxes and energy-angular distributions of H+ and He++ around the Sun direction with high time resolution.\nZ.NEMECEK, Ya.SAFRANKOVA, Charles Univ., Prague, Czech. Republic - A.FEDOROV, G.ZASTENKER IKI, Moscow, Russia\n\nCORAL\nAngular/energy ion distributions at all directions in energy range 0.05-25 ke V/Q\nR.JIMENEZ INTERCOSMOS, Havana, Cuba - O.VAISBERG, Yu.YERMOLAEV IKI, Moscow, Russia\n\nALPHA-3\nThermal plasma ion flux E < 25 eV/Q\nV.BEZRUKIKH IKI, Moscow, Russia\n\nWAVES AND FIELDS\n\nASPI\nFields and waves consortium (Analysis of Spectra of Plasma waves and Instabilities, including MIF-M, OPERA, ADS, IFPE, FGM-I, KEM-3, PRAM).\nS.KLIMOV, S.ROMANOV IKI, Moscow, Russia\n\nOPERA\nThree-component electric field fluctuations in the range 0-50 kHz including spectral analysis. \nFGM-1 magnetic field data acquisition and processing.\nE.AMATA CNR/IFSI, Frascati, Italy - S.SAVIN IKI, Moscow, Russia - R.GRARD SSD/ESTEC, ESA - J.L.RAUCH LPCE (now LPC2E), Orleans, France\n\nMIF-M\nDC/AC magnetic field, 3 components, 0-64 Hz, 1 component, 1 Hz - 40 kHz. Data are processed for SSNI by PRAM.\nS.ROMANOV, M.NOZDRACHEV IKI, Moscow, Russia - V.KOREPANOV SDD ASU, Lvov, Ukraine\n\nIFPE\nMeasurements of ion and electron flux fluctuations in the range 0.1 Hz - 1 kHz, the data are processed for SSNI by PRAM.\nJ.BUCHNER MPE-A, Berlin, Germany - S.ROMANOV IKI, Moscow, Russia\n\nADS\nNine-channel spectra-analyzer and cross-correlator, two-component measurements of current fluctuations, 0.1 Hz - 40 kHz.\nJ.JUCHNIEWICZ Space Res. Center, Warsaw, Poland - L.WOOLLISCROFT Departm. of Contr. Engineering Sheffield Univ, Sheffield, UK - S.KLIMOV IKI, Moscow, Russia - V.KOREPANOV SDD ASU, Lvov, Ukraine\n\nFGM-1\nMeasurements of 3D magnetic field 0-25 Hz in the range 0.25-256 nT. OPERA acquires and processes the data for SSNI.\nJ.RUSTENBACH MPE-A Berlin, Germany - S.SAVIN IKI, Moscow, Russia\n\nKEM-3 (aboard subsatellite)\nElectric (0.1 Hz - 400 kHz) and magnetic (1-50 kHz) fields, two-component measurements of current fluctuations 0.1 Hz - 40 kHz.\nP.TRISKA, F.JIRICEK Inst. Atm. Phys. CAS, Prague, Czech., Republic - S.KLIMOV IKI, Moscow, Russia\n\nPRAM\nDC/AC magnetic field from MIF-M, ion and electron flux from IFPE data processor and RF-15-1 data processor.\nS.ROMANOV (ASPI), O.LIKIN (RF-15-I) IKI, Moscow, Russia - F.FARNIK Astr. Inst. CAS, Ondrejov, Czech. Republic.\n\nFM-3I\nMagnetic field (three components). Range : 0.2-200 nT,  0.5-1000nT. Band : 0-10 Hz\nM.NOZDRACHEV IKI, Moscow, Russia - V.STYAZHKIN IZMIRAN, Troitsk, Russia\n\nAKR-X\nRadioemission in the range 100 kHz - 1.5 MHz\nL.FISCHER Komensky University, Bratislava, Slovakia - V.GRIGORIEVA Astron. Inst. of Moscow University, Moscow, Russia\n\nENERGETIC PARTICLES\n\nSKA-2\nCharged energetic particles (Ee = 40-200 keV, Ei = 0.05-150 keV) composition and anizotropy\nE.MOROZOVA, E.BUDNIK, IKI, Moscow, Russia - S.FISCHER Astronomical Institute, Prague, Czech. Republic - E.SARRIS University of Thrace, Xanthi, Greece\n\nDOK-2\nEnergy spectra, angular distributions and time variations of electrons (E = 15-400 keV) and ions (E = 20-1000 keV)\nK.KUDELA Institute of Experim. Physics. SAS, Kosice, Slovakia - V.LUTSENKO IKI, Moscow, Russia - E.SARRIS, University of Thrace, Xanthi, Greece\n\nRF-15-I\nSolar X-ray burst spectra and time profile measurements in the range 2-240 keV, The data are processed by PRAM.\nO.LIKIN IKI, Moscow, Russia - F.FARNIK Astr. Inst. CAS, Ondrejov, Czech. Republic - J.SYLVESTER Space Res. Center, Wroclaw, Poland\n\nSOSNA-3\nDosimetric measurements\nV.BENGIN, V.PETROV IMBP, Moscow, Russia - S.KUZNETSOV Moscow University, Moscow, Russia\n\nRKI-2\nIonizing radiation (5, 15, 40, 100, 500 MeV) and UV radiation from the Sun.\nT.KAZACHEVSKAYA IPG, Moscow, Russia\n\nSERVICE SYSTEMS\n\nBNK, BNTR, BNTS\nCommutation blocks\nT.LESSINA IKI, Moscow, Russia\n\nSSNI\nTelemetry system\nL.CHESALIN IKI, Moscow, Russia\n\nSTO\nTransmitter for the interferometric measurements\nJ.VOITA Inst. Atm. Phys. CAS, Prague, Czech. Republic - G.TEREKHIN IKI, Moscow, Russia\n\nBNS\nAttitude processor\nJ.KLAS Inst. Atm. Phys. CAS, Prague, Czech. Republic - N.EISMONT, Yu.LISSAKOV IKI, Moscow, Russia",
        "Contact": {
          "PersonID": "spase://CNES/Person/CDPP-Archive/Lev.Zelenyi",
          "Role": "ProjectScientist"
        }
      },
      "ObservatoryGroupID": "spase://CNES/Observatory/CDPP-Archive/Interball",
      "Location": {
        "ObservatoryRegion": "Heliosphere.NearEarth"
      },
      "OperatingSpan": {
        "StartDate": "1995-08-03T00:00:00Z",
        "StopDate": "2000-10-16T00:00:00Z"
      }
    }
  }
}