CategorySolar: Maximum Mission Wikimedia Commons.
Jump to navigation Jump to search. Solar Maximum Mission it; Solar Maximum Mission fr; Solar Maximum Mission ca; Solar Maximum Mission de-ch; Solar Maximum Mission de; Solar Maximum Mission pt; Solar Maximum Mission en-gb; zh; zh-hans; zh-hk; Solar Maximum Mission pt-br; Solar Maximum Mission es; Solar Maximum Mission lb; Solar Maximum Mission pl; Solar Maximum Mission nb; Solar Maximum Mission nl; zh-hant; ar; Solar Maximum Mission en; ja; Solar Maximum Mission gl; Solar Maximum Mission en-ca; Solar Maximum Mission cs; SMM ru space observatory en Solar Maximum Mission ru; SolarMax de; Solar Max, Solarmax fr; SolarMax en; Solar Max pl; SolarMax, SMM cs; SMM es.
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April 11, 1984: Shuttle Makes House Call, Repairs Satellite WIRED. Menu. Story Saved. Close. Chevron. Story Saved. Close. Search. Facebook. Twitter. Email. Save Story. Facebook. Twitter. Email. Save Story. Facebook. Twitter. Pinterest. YouTube. Instagram.
April 11, 1984: Shuttle Makes House Call, Repairs Satellite. 1984: Shuttle astronauts retrieve the malfunctioning Solar Max astronomy satellite, fix it and send it back into orbit. Its the first time a satellite has been repaired in space. The Solar Maximum mission had been launched Feb.
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Solar Maximum Mission United States space laboratory Britannica.
Solar Maximum Mission SMM satellite during an in-orbit repair mission by the crew of Space Shuttle Challenger in April 1984. The SMM satellite is specially equipped to observe the Sun in white light through the gamma-ray region of the electromagnetic spectrum and to monitor its total energy output.
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SMM - eoPortal Directory - Satellite Missions.
6 NASA's' Solar Maximum Mission: A Look at the New Sun, June 1987, NASA brochure, edited by J. 7 The Solar Maximum Mission Experiments, Solar Physics, Volume 65, pp. 10 Chris St.Cyr, Joan Burkepile, Solar Maximum Mission Overview, URL: http://smm.hao.ucar.edu/smm/smm_mission.html.:
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Solar Maximum Mission SMM UCL Department of Space and Climate Physics - UCL - University College London.
UCL Department of Space and Climate Physics. Solar Maximum Mission SMM. Solar Maximum Mission SMM. X-ray Polychromator XRP designed to investigate Solar phenomena - 1980. 14 February 1980. The Solar Maximum Mission satellite or SolarMax was designed to investigate Solar phenomena, particularly solar flares.
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High-energy flare observations from the Solar Maximum Mission Philosophical Transactions of the Royal Society of London. Series A: Physical and Engineering Sciences.
Published: 16 September 1991 https://doi.org/10.1098/rsta.1991.0086.: We review high-energy observations of solar flares with emphasis on measurements by instruments on the Solar Maximum Mission satellite. Those observations show that, contrary to prior expectation, high-energy emission is a common property of solar flares.
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New Results from the Solar Maximum Mission/Bent Crystal Spectrometer SpringerLink.
The Bent Crystal Spectrometer BCS onboard the NASA Solar Maximum Mission was part of the X-ray Polychromator, which observed numerous flares and bright active regions from February to November 1980, when operation was suspended as a result of the failure of the spacecraft fine-pointing system.
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SMM eoPortal Directory Satellite Missions.
Chaikin, Solar Max: Back from the Edge, Sky Telescope, June 1984, pp. Withbroe, Solar Maximum Mission, Solar Physics, Vol. 65, No 1, Feb. 6 NASA's' Solar Maximum Mission: A Look at the New Sun, June 1987, NASA brochure, edited by J.
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NASA/Marshall Solar Physics.
The Solar Maximum Mission SMM or SolarMax was launched on February 14, 1980. It carried several scientific instruments which provided new insights into the nature of solar flares. The spacecraft was rescued and repaired by a 1984 Space Shuttle Challenger mission.
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Observations from the Solar Maximum Mission on JSTOR.
jstor org stable/53820. After nearly a decade of flare observations from the Solar Maximum Mission SMM, the time has come to pause to review what has been accomplished and to identify the problems that remain to be solved. SMM has not only produced a comprehensive database on a variety of active-Sun phenomena but also taught us how to coordinate observations with ground-based observatories and other spacecraft to produce a more holistic view of the complex energy release and transport processes that we call a flare.
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