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The strong radio emission on July 10 at all wavelengths occurred about 25 min after the SXR maximum (M5.7), which was 20 times as strong as that before the SXR maximum which triggered the flare. The fine structures in 1-2 GHz may be interpreted by SQM, and further effort is needed.

 

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Responsible NASA Official:  Gordon D. Holman

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Heliophysics Science Division
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Gordon.D.Holman@nasa.gov

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This site last updated November 10, 2008.