The Vertical Structure of Dynamo Winds Deduced from Geomagnetic Variations Associated with Solar Flares

The Vertical Structure of Dynamo Winds Deduced from Geomagnetic Variations Associated with Solar Flares

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A detailed time analysis of the massive solar flare that occurred at 1522 UT on 28 August 1966 and a study of its implications for the large-scale wind system in the 90-140 km dynamo region of the atmosphere.