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SME
Solar Mesosphere Explorer
SME was developed to investigate the processes that create and destroy ozone in the Earth's upper atmosphere. The mission's specific goals were to examine (1) the effects of changes in the solar ultraviolet flux on mesospheric ozone densities, (2) the relationship between solar flux, ozone, and the temperature of the upper stratosphere and mesosphere, (3) the relationship between ozone and water vapor, and (4) the relationship between nitrogen dioxide and ozone. Contact was lost on April 14, 1989 after a battery failure, and the vehicle reentered on March 5, 1991. The mission was managed for NASA by JPL, and was operated by the Laboratory for Atmospheric and Space Physics of the University of Colorado.
Spacecraft
Spin stabilized (~5 rpm). Fixed solar array. Tape recorder. NiCd batteries. The spacecraft
was controlled from University of Colorado's Laboratory for Atmospheric and Space
Physics (LASP) in Boulder via NASA, GSFC.
Payload
Ultraviolet ozone spectrometer. 1.27 micron spectrometer. Nitrogen dioxide spectrometer.
Four-channel infrared radiometer. Solar ultraviolet monitor. Solar proton alarm detector. All instruments were turned off in December, 1988 due to power constraints.
Country of Origin | United States |
Customer/User | NASA, NOAA, NCAR, LASP (Univ. of Colo.) |
Manufacturer(s) | JPL, Ball Space Systems |
Size | 1.25 m diameter x 1.7 m high cylinder |
Orbit | 538 x 542 km, incl. = 97 deg, 3 a.m. - 3 p.m. sun-synchronous |
Design Life | 1 year |
Launch Facts
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Name | Int'l Desig. | Date | Site | Vehicle | Orbit | Mass(kg) |
Notes |
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SME | 1981-100A | 10/6/81 | WSMC | Delta 2310 | LEO | 437 |
Solar Mesosphere Explorer |
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