Influence of photospheric parameters on solar spectral line parameters.

Astronomy and Astrophysics – Astronomy

Scientific paper

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Solar Photosphere: Spectral Lines

Scientific paper

Spectral line profiles for 31 solar spectral line from the Belgrade observational program have been synthesized previously. The authors gave a short review on the sensivity of those spectral lines examining the behaviour of some line profile parameters (equivalent width, central residual flux, full-half width) induced by independent variations of temperature, gas pressure and electron density gradient in the atmosphere model. The results displayed as gradients of line profile parameters have shown high sensitivity of spectral lines to the temperature and a negligible sensitivity to the pressure and electron density change.

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