Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003padeu..13...81k&link_type=abstract
In: Contributions to NATO Advanced Research Workshop Turbulence, Waves, and Instabilities in the Solar Plasma; Hungary, 16-20 Se
Astronomy and Astrophysics
Astronomy
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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