For over 10 years, the instruments carried on the satellite, including the Canadian-built suprathermal ion mass spectrometer (SMS), have measured magnetic and electrical fields, plasma, and waves.
Ion-composition measurements from the suprathermal mass spectrometer (SMS) on AKEBONO (EXOS-D) during large magnetic storms (minimum Dst < −50 nT) reveal substantial changes in the mass composition of the auroral ionosphere.
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Launch from ISAS range in Kagoshima of Japan's EXOS-D science satellite (renamed Akebono after reaching orbit), carrying a Canadian-built instrument, the suprathermal ion mass spectrometer.
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February 22 Launch from ISAS range in Kagoshima of Japan's EXOS-D science satellite (renamed Akebono after reaching orbit), carrying a Canadian-built instrument, the suprathermal ion mass spectrometer.
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CLICK TO ENLARGE More specifically, the ePOP instruments are: the Imaging Rapid-scanning Ion Mass Spectrometer (IRM); the Suprathermal Electron Imager (SEI); the Magnetic Field Instrument (MGF); the Fast Auroral Imager (FAI); the Radio Receiver Instrument (RRI); the Neutral Mass and Velocity Spectrometer (NMS); the GPS Attitude and Positioning Experiment (GAP); and the Coherent Electromagnetic Radiation (CER).