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Flare-produced coronal waves

Published online by Cambridge University Press:  14 August 2015

Friedrich Meyer
Friedrich Meyer*
Affiliation:
Max-Planck-Institut für Physik und Astrophysik, München, Germany

Abstract

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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 

References

Moreton, G.E., (1960) Astronom. J., 65, 494.Google Scholar
Moreton, G.E., (1965) in Stellar and Solar Magnetic Fields. I.A.U. Symp. 22, North-Holland Publishing Co., Amsterdam, p. 371.Google Scholar
Zirin, H. (1966) The Solar Atmosphere, Blaisdell Publishing Co., Waltham, Mass., p. 400ff, Fig. 13.11 and 13.12.Google Scholar