Electron-Density Fluctuations

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

On the basis of quasi-hydrodynamic equations we consider formation of electron-density fluctuations by turbulent mixing of weakly-ionized plasma in the solar atmosphere. An expression for the power spectrum of the fluctuations is obtained, assuming quasi-neutrality and isothermality. The expression is used to predict the shape of the spatial spectrum and the rms level of the plasma fluctuations in the lower part of the solar atmosphere.

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