Statistics – Computation
Scientific paper
Feb 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989arb..nasa..107t&link_type=abstract
In its Annual Research Briefs, 1988 p 107-114 (SEE N89-22817 16-34)
Statistics
Computation
Angular Momentum, Mass Transfer, Mathematical Models, Solar Corona, Stellar Evolution, Turbulence, Turbulent Heat Transfer, Channel Flow, Compressible Flow, Dissipation, Energy Spectra, Reynolds Stress, Solar System, Tensors, Turbulent Flow
Scientific paper
It is likely that turbulence played a major role in the evolution of the solar nebula, which is the flattened disk of dust and gas out of which our solar system formed. Relevant turbulent processes include the transport of angular momentum, mass, and heat, which were critically important to the formation of the solar system. This research will break ground in the modeling of compressible turbulence and its effects on the evolution of the solar nebula. The computational techniques which were developed should be of interest to researchers studying other astrophysical disk systems (e.g., active galactic nuclei), as well as turbulence modelers outside the astrophysics community.
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