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Modelling a Solar Flare from X-UV and Radio Observations
Published online by Cambridge University Press: 19 July 2016
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A slow evolving flaring loop has been observed by the UVSP, XRP and HXIS instruments on board SMM on June 10, 1980. Simultaneous radio observations from Toyokawa (Japan) are also available. The former instruments have an angular resolution ranging from 3“ to 30“ which allows the determination of the loop structure. The XRP:FCS rasters permit to analyze the flare only during three time intervals of about 10 minutes each.
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- VIII. Solar Flares
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- Copyright © Kluwer 1990
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