astronomical > morn Satellites
Contents
No. 1
  Sunrise Satellite (hinode) is one from Japan, the United Kingdom and the United States jointly developed solar observation satellite, formerly known as solar-b, on September 22, 2006 in Kyushu, Japan's Uchinoura Space Center launch. Sunrise satellites in nearly circular sun-synchronous orbit and a perigee of 280 km and an apogee of 686 km. The satellite's main purpose is to observe the fine structure of the solar magnetic field to study solar flares and other violent activities of the outbreak of shooting high quality pictures of the sun.
  The main satellite on board scientific instruments are:
  Solar Optical Telescope (sot), diameter of 0.5 meters, with a vector magnetic imager, the spatial resolution of 0.2 arc seconds.
  x-ray telescope (xrt), diameter 34 cm grazing incidence telescope, using the Walter type Ⅰ light path.
  Extreme Ultraviolet Imaging Spectrograph (eis).
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No. 2
  Sunrise Satellite (Hinode) is one from Japan, the United Kingdom and the United States jointly developed solar observation satellite, formerly known as Solar-B, on September 22, 2006 in Kyushu, Japan's Uchinoura Space Center launch. Sunrise satellites in nearly circular sun-synchronous orbit and a perigee of 280 km and an apogee of 686 km. The satellite's main purpose is to observe the fine structure of the solar magnetic field to study solar flares and other violent activities of the outbreak of shooting high quality pictures of the sun.
  The main satellite on board scientific instruments are:
  Solar Optical Telescope (SOT), diameter of 0.5 meters, with a vector magnetic imager, the spatial resolution of 0.2 arc seconds.
  X-ray Telescope (XRT), diameter 34 cm grazing incidence telescope, using the Walter type Ⅰ light path.
  EUV Imaging Spectrometer (EIS).
Translated by Google