The energy of waves in the photosphere and lower chromosphere - IV. Inversion results of Ca II H spectra

@inproceedings{Beck2013TheEO,
  title={The energy of waves in the photosphere and lower chromosphere - IV. Inversion results of Ca II H spectra},
  author={C. Beck and Reza Rezaei and Klaus Gerhard Puschmann},
  year={2013}
}
Context. Most semi-empirical static one-dimensional (1D) models of the solar atmosphere in the magnetically quiet Sun (QS) predict an increase in temperature at chromospheric layers. Numerical simulations of the solar chromosphere with a variable degree of sophistication, i.e. from 1D to three-dimensional (3D) simulations; assuming local thermal equilibrium (LTE) or non-LTE (NLTE), on the other hand, only yielded an increase in the brightness temperature without any stationary increase in the… CONTINUE READING

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