Modelling a solar flare from X-ray, UV,
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F. Chiuderi Drago; B. C. Monsignori Fossi
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Article
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1991
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Springer
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English
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A slowly evolving, flaring loop was observed by the UVSP, XRP, and HXIS instruments onboard SMM on June 10, 1980. Simultaneous radio observations from Toyokawa (Japan) are also available. The SMM instruments have an angular resolution ranging from 3 to 30 arc sec by which the loop structure may be d