Turbulence in circumstellar discs

Details Turbulence in circumstellar discs Turbulence in circumstellar discs

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.175..261h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 175, no. 2, Jan. 1991, p. 261-281.

Statistics

Computation

3

Stellar Envelopes, Turbulent Flow, Computational Astrophysics, Equations Of State, Equilibrium Equations, High Temperature Gases, Temperature Distribution

Scientific paper

A statistical model for the small-scale turbulence of circumstellar
disks yields equations which in stationary systems are mathematically
equivalent to those of partially elastic impacts, although the physical
content is different. The disk is turbulent but not convective on this
scale.

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