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Solar Radiation and Thermospheric Satellite

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Solar Radiation and Thermospheric Satellite (SRATS), also knows as Taiyo ("Sun" in Japanese) or Shinsei-3,[1] was a space probe developed by the Institute of Space and Astronautical Science (ISAS) at the University of Tokyo. Launched on February 24, 1975, from Kagoshima Space Center by M-3C-2 rocket, its mission focused on studying upper atmospheric physics, X-ray and UV solar radiation, and the Earth's ionosphere. Taiyo completed its mission before re-entering Earth's atmosphere on June 29, 1980.[2]

The satellite had a shape of octagonal cylinder (or prism), weighing 86 kg. It orbited the Earth in an elliptical orbit with a periapsis of 260 km and an apoapsis of 3,140 km, at a 32-degree inclination. The satellite's primary goal was to investigate solar X-rays, ultraviolet radiation, and the distribution of ions and electrons in the Earth’s upper atmosphere.[2][3]

Instruments

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Taiyo had seven science instuments:[2]

  • Solar X-Ray Detector (SXR): Designed to observe solar X-rays in two energy ranges (5.9-9.5 keV, 9.5-11.5 keV) and measure charged particles near the Earth's radiation belts.
  • Lyman-alpha Radiation Monitor (SXU): Measured solar hydrogen Lyman-alpha radiation to study the Sun's chromosphere.
  • Geocoronal and Middle Ultraviolet Radiometers (GMV): This system combined the Middle Ultraviolet Radiometer (MUV), which measured reflected solar light from atmospheric ozone, and the Vacuum Ultraviolet Photon Counter (GUV), which analyzed geocoronal emissions.
  • Bennett Ion Mass Spectrometer (CPI): Examined ion composition in the upper atmosphere, identifying H+, He+, and O+ ions.
  • Retarding Potential Analyzer (RPA): Measured ion density and temperature using voltage sweeps across ion traps.
  • Electron Temperature Probe (TEL): Recorded electron temperature variations, capable of measuring up to 4000 K.
  • Gyro-Plasma Probe (IMP): Analyzed electron density distribution through high-frequency impedance measurements.

Further reading

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  • Hirao, Kunio (1975). "The TAIYO Mission". J.Geomag,Geoelectr. 27: 265–270. Retrieved 22 October 2024.
  • Hirao, K. (1 January 1976). "Results of observations made by the SRATS (solar radiation and thermospheric structure) satellite". Retrieved 22 October 2024. {{cite journal}}: Cite journal requires |journal= (help)
  • Matsuoka, Masaru; Nagai, Fukuo; Ohki, Ken-ichiro (1975). "A solar X-ray detector aboard "TAIYO"". Journal of geomagnetism and geoelectricity. 27 (4): 271–277. doi:10.5636/jgg.27.271.
  • Oshio, Takanori; Masuoka, Toshio; Higashino, Ichiro; Watanabe, Norihiko (1975). "An intensity monitor for solar hydrogen Lyman-.ALPHA. radiation (TAIYO SXU)". Journal of geomagnetism and geoelectricity. 27 (4): 279–294. doi:10.5636/jgg.27.279.
  • Tohmatsu, Takao; Suzuki, Katsuhisa; Ogawa, Toshihiro (1975). "The atmospheric UV instrumentation for the satellite "TAIYO"". Journal of geomagnetism and geoelectricity. 27 (4): 295–301. doi:10.5636/jgg.27.295.
  • Iwamoto, Iwao; Suitz, Takeshi; Fugono, Nobuyoshi (1975). "The Bennett ion mass spectrometer aboard "TAIYO" (CPI)". Journal of geomagnetism and geoelectricity. 27 (4): 303–310. doi:10.5636/jgg.27.303.
  • Miyazaki, Shigeru (1975). "The retarding potential analyzer aboard the satellite TAIYO". Journal of geomagnetism and geoelectricity. 27 (4): 311–320. doi:10.5636/jgg.27.311.
  • Oyama, Koh-ichiro; Hirao, Kunio (1975). "Electron temperature probe experiments on the satellite "TAIYO"". Journal of geomagnetism and geoelectricity. 27 (4): 321–330. doi:10.5636/jgg.27.321.
  • Oya, Hiroshi; Morioka, Akira (1975). "Instrumentation and observations of gyro-plasma probe installed on TAIYO for measurement of ionospheric plasma parameters and low energetic particle effects". Journal of geomagnetism and geoelectricity. 27 (4): 331–361. doi:10.5636/jgg.27.331.

References

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  1. ^ Darling, David. "Taiyo". www.daviddarling.info. Retrieved 22 October 2024.
  2. ^ a b c "DARTS for Astrophysics". DARTS at ISAS/JAXA. Retrieved 22 October 2024.
  3. ^ "TAIYO | Spacecraft". ISAS. Retrieved 22 October 2024.