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Flare-produced coronal waves
Published online by Cambridge University Press: 14 August 2015
Abstract
We present a coronal propagation model for fast chromospheric disturbances following flares that were first observed by Moreton and Ramsey, and deduce estimates of average coronal magnetic fields (6 gauss) and disturbance energies (≤ 1029 erg).
- Type
- Part VI: Transient Phenomena
- Information
- Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 485 - 489
- Copyright
- Copyright © Reidel 1968
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