{
  "Spase": {
    "xmlns": "http://www.spase-group.org/data/schema",
    "xmlns:xsi": "http://www.w3.org/2001/XMLSchema-instance",
    "xsi:schemaLocation": "http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_4_0.xsd",
    "Version": "2.4.0",
    "Observatory": {
      "ResourceID": "spase://CNES/Observatory/CDPP-Archive/Interball-Auroral",
      "ResourceHeader": {
        "ResourceName": "Interball-Auroral",
        "ReleaseDate": "2022-04-28T17:46:51Z",
        "Description": "The AURORAL PROBE with its subsatellite was launched on 29 August 1996, also to the 65 degrees inclination orbit, but with the apogee of 20 000 km above the northern auroral zone and polar cap.\nTwo different auroral imagers are installed on the Auroral probe main satellite. These imagers are aimed to provide the two-dimensional global patterns of auroral phenomena and their time development. This allows to place in situ measurements from the two probes in the global geophysical perspective of large-scale magnetospheric processes.\n\nInterball Auroral Probe : On-board Experiments\n\nPLASMA\n\nSKA-3\nSpectra of electrons and ions 0.03 < E < 15 keV, Anisotropy of electrons and ions (M = 1, 4, 16),  30 < E < 500 keV/Q\nYu.GALPERIN, R.KOVRAZHKIN, A.KUZMIN, F.SHUISKAYA IKI, Moscow, Russia\n\nION\nElectron and ion spectra and anisotropy (M = 1, 2, 4, 16),  0.005 < E < 20 keV/Q\nJ.A.SAUVAUD CESR, Toulouse, France - R.A.KOVRAZHKIN, K.AFANASIEV IKI, Moscow, Russia\n\nPROMICS-3\nIon composition (M = 1-32) and 3-D energy distribution 10 eV < E < 30 keV/Q\nI.SANDAHL IRF, Kiruna, Sweden - N.PISSARENKO, E.DUBININ IKI, Moscow Russia - H.KOSKINEN, T.PULKKINEN FMI, Helsinki, Finland\n\nTHERMAL PLASMA\n\nHYPERBOLOID\nIon composition and 3-D distribution functions M = 1-32 (with H+, He+, O++, O+ routinely), 0.1 < E < 80 eV\nJ.J.BERTHELIER CETP Saint Maur, France - Yu.GALPERIN, T.MULIARCHIK IKI, Moscow, Russia\n\nKM-7\nTemperature of cold electrons T < 10 eV\nJ.SMILAUER Inst. of Atm. Physics. CAS, Prague, Czech. Republic - V.AFONIN IKI, Moscow, Russia\n\nALPHA-3\nThermal plasma ion flux E < 25 eV/Q\nV.BEZRUKIKH IKI, Moscow, Russia\n\nWAVES AND FIELS\n\nIMAP-3\nMagnetic field (three components) Range 1 ÷ ± 70 000 nT, band 0-10 Hz\nI.ARSHINKOV SDS, Sofia, Bulgaria - L.ZHUZGOV, V.STYAZHKIN IZMIRAN, Troitsk, Russia\n\nIESP-2M\nDC electric field and ULF waves (0.1-30 Hz)\nS.PERRAUT CETP Velizy, France - M.MOGILEVSKY IKI, Moscow, Russia\n\nPOLRAD\nAuroral Kilometric radiation (4 kHz - 2 MHz)\nJ. HANASZ, (Space Res. Centre PAS - Torun, Poland) - R. SCHREIBER (Copernicus Astr. Centre PAS - Torun, Poland) - H. DE FERAUDY (CETP/CNRS - Velizy, France)\n\nMEMO\nElectromagnetic waves in wide band (quantitative analysis) < 240 kHz\nF.LEFEUVRE LPCE Orleans, France - M.MOGILEVSKY IKI, Moscow, Russia\n\nNVK-ONCH\nVLF electromagnetic waves 20 Hz - 20 kHz\nA.GOLJAVIN IZMIRAN, Troitsk, Russia - M.MOGILEVSKY IKI, Moscow, Russia\n\nENERGETIC PARTICLES\n\nDOK-2\nEnergy spectra, angular distributions and time variations of electrons (E = 20-1000 keV)\nK.KUDELA Inst. of Experim. Phys. SAS, Kosice, Slovakia - V.LUTSENKO IKI, Moscow, Russia - E.SARRIS University of Thrace, Xanthi, Greece\n\nS/C POTENTIAL CONTROL\n\nRON\nSpace electric potential control by two ion beams (N2+, In+). Ion beam currents Ibeam = 0-15 µA\nW.RIEDLER, K.TORKAR Space Res. Inst. Austrian Acad. Sci., Graz, Austria - R.SCHMIDT ESA/ESTEC, Nordwijk, The Netherlands - Yu.GALPERIN, M.VESELOV IKI, Moscow, Russia\n\nOPTICAL OBSERVATIONS\n\nUVAI\nUV auroral imager (140 - 160 nm)\nL.COGGER Univ. of Calgary, Canada - Yu.GALPERIN, M.VESELOV IKI, Moscow, Russia\n\nUVSIPS\nUV auroral oxygen emissions 130.4, 135.6, 149.3 nm in the footprint region of the Earth's atmosphere\nA.KUZMIN IKI, Moscow, Russia - K.PALAZOV Observ. Yuri Gagarin, Stara Zagora, Bulgaria\n\nTECHNOLOGICAL EXPERIMENTS\n\nRD-1M\nDosimetric measurements\nV.BENGIN, V.PETROV IMBP, Moscow, Russia - S.KUZNETSOV Moscow University, Moscow, Russia\n\nANOD\nComparison of different models of solar panels\nA.KOZLOV State Scientific-industrial corporation QVANT, Moscow, Russia - T.MULIARCHIK IKI, Moscow, Russia\n\nSERVICE SYSTEMS\n\nBNK, BNTR, BNTS\nCommutation blocks\nJ.DIKAREVA IKI, Moscow, Russia\n\nSSNI\nTelemetry system\nL.CHESALIN IKI, Moscow, Russia\n\nSTO\nTelemetry system\nL.BODNAR Politechn. Inst., Budapest, Hungary - J.VOJTA Inst. of Atm. Phys. CAS, Prague, Czech. Republik - S.ROISHIK Aviation Inst., Warsaw, Poland - G.TEREKHIN IKI, Moscow, Russia\n\nBNS\nAttitude processor\nJ.KLAS Inst. of 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",
          "Earth.Magnetosheath",
          "Earth.Magnetosphere",
          "Earth.Magnetosphere.Main",
          "Earth.Magnetosphere.Polar"
        ]
      },
      "OperatingSpan": {
        "StartDate": "1996-08-29T00:00:00Z",
        "StopDate": "1999-01-26T00:00:00Z"
      }
    }
  }
}