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Hα Fine Structure and the Dynamics of the Solar Atmosphere

Published online by Cambridge University Press:  14 August 2015

Franz-Ludwig Deubner
Franz-Ludwig Deubner*
Affiliation:
Fraunhofer Institut, Freiburg, G.F.R.

Abstract

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Series of simultaneous spectra in different spectral regions, representing all ‘visible’ layers of the solar atmosphere, of high spatial and temporal resolution are used to compute power spectra and diagnostic diagrams of intensity and velocity fluctuations in order to study the dynamic response of the chromosphere to disturbances from below.

Type
Part VI: Evolution of Chromospheric Fine Structures
Information
Symposium - International Astronomical Union , Volume 56: Chromospheric Fine Structure , 1974 , pp. 263 - 266
Copyright
Copyright © Reidel 1974