Density fluctuations in the solar wind : effects of nearly incompressible theory

Details Density fluctuations in the solar wind : effects of nearly incompressible theory Density fluctuations in the solar wind : effects of nearly incompressible theory

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsh23a1136h&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SH23A-1136

Physics

2164 Solar Wind Plasma, 7863 Turbulence (4490)

Scientific paper

Previously derived nearly incompressible theory with the inclusion of a simple large-scale inhomogeneous background (static and spherically symmetric) is examined by direct numerical simulations of non-stationary two dimensional turbulence. According to the theory, leading order density fluctuations satisfy a passive scalar evolution equation with additional source term induced by coupling to the large-scale inhomogeneous background. In this poster we investigate the decay rates and spectral shapes of density fluctuations together with implications for solar wind data.

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