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Hα Fine Structure and the Dynamics of the Solar Atmosphere
Published online by Cambridge University Press: 14 August 2015
Abstract
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
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