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Solar Intensity X-ray and particle Spectrometer (SIXS)

✍ Scribed by J. Huovelin; R. Vainio; H. Andersson; E. Valtonen; L. Alha; A. Mälkki; M. Grande; G.W. Fraser; M. Kato; H. Koskinen; K. Muinonen; J. Näränen; W. Schmidt; M. Syrjäsuo; M. Anttila; T. Vihavainen; E. Kiuru; M. Roos; J. Peltonen; J. Lehti; M. Talvioja; P. Portin; M. Prydderch


Book ID
108255759
Publisher
Elsevier Science
Year
2010
Tongue
English
Weight
861 KB
Volume
58
Category
Article
ISSN
0032-0633

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The primary scientific objectives of the Hard X-Ray Burst Spectrometer (HXRBS) to be flown on the Solar Maximum Mission are as follows: (1) To determine the nature of the mechanisms which accelerate electrons to 20-100 keV in the first stage of a solar flare and to > 1 MeV in the second stage of man