Generation of Atmospheric Turbulence by Solar Radiation

Details Generation of Atmospheric Turbulence by Solar Radiation Generation of Atmospheric Turbulence by Solar Radiation

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..88..205v&link_type=abstract

Astrophysics and Space Science, Volume 88, Issue 1, pp.205-217

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

A statistical framework of weak turbulence is applied to investigate the maintenance of atmospheric turbulence during a long period, even after the external energy supply from solar radiations has stopped. Thus, the problem of hydrodynamical turbulence without any mean motion is dealt with. Main attention is drawn to one-dimensional Burgers equation, together with a discussion devoted mainly to Millionshtchikov's hypothesis, which may be applied as a consequence of the assumed weak turbulence. Remarkably, this leads to an explicit proof of the existence of the ‘cascade process’ in turbulence. The results are illustrated by numerical calculations.

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