PastHINOTORI

The Solar Observation Satellite “HINOTORI” aims to observe of 2D data in hard X-ray of solar flares, solar particle rays, X-ray bursts, etc.

TENMA TANSEI-4
Name (pre-launch in parentheses) HINOTORI (ASTRO-A)
International Designation code 1981-017A
Objectives Observation of 2D data in hard X-ray of solar flares, solar particle rays, X-ray bursts, etc.
Launch Date 09:30, February 21, 1981 (JST)
Launch Location Kagoshima Space Center (Uchinoura)
Launch Vehicle M-3S-2
Weight 188kg
Shape Octagonal cylinder, 92.8 cm long from face to face, 81.5 cm high
Equipped with four solar-array paddles
Orbital Altitude Perigee 576 km, Apogee 644 km
Orbital Inclination 31°
Type of orbit Near-circular
Orbital Period 97 min
Scientific Instruments 1.Solar flare X-ray imager (SXT)
2.Solar soft X-ray bright line spectrum analyzer (SOX)
3.Solar soft X-ray monitor (HXM)
4.Solar flare monitor (FLM)
5.Solar gamma ray monitor (SGR)
6.Particle ray monitor (PXM)
7.Plasma electron density measurement instrument (IMP)
8.Plasma electron temperature measurement instrument (TEL)
End of Operation July 11, 1991
Reentered Date July 11, 1991
Results In addition to its own mission, HINOTORI also provided observational data to the international project on the maximum period of solar activity. On the first day after the start of normal operation, it observed a large solar flare and, a month later, succeeded in observing 41 flares of many sizes. With the satellite’s X-ray observations, we were able to discover several new facts including high-temperature phenomena reaching up to 50 million °C and clouds of light-speed electrons floating in coronas