The energy of waves in the photosphere and lower chromosphere. II. Intensity statistics
Context. The energy source powering the solar chromosphere is still undetermined, but leaves its traces in observed intensities. Aims: We investigate the statistics of the intensity distributions as a function of the wavelength for Ca ii H and the Ca ii IR line at 854.2 nm to estimate the energy content in the observed intensity fluctuations
Beck, C. et al.
Fecha de publicación:
8
2012