Oceanic and interstellar Fossil turbulence

Details Oceanic and interstellar Fossil turbulence Oceanic and interstellar Fossil turbulence

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aipc..174...74g&link_type=abstract

IN: Radio wave scattering in the interstellar medium; Proceedings of the AIP Conference, San Diego, CA, Jan. 18, 19, 1988 (A89-2

Physics

1

Gravitational Effects, Interstellar Matter, Magnetohydrodynamic Turbulence, Stratified Flow, Gravitational Collapse, Gravitational Fields, Hypersonic Flow, Interstellar Magnetic Fields

Scientific paper

Turbulence in the stratified ocean is inhibited at large scales by gravity, leaving internal waves and partially mixed fluctuations in the density field called fossil turbulence. Information about previous turbulence activity is preserved by the fossil remnants of three- and possibly two-dimensional turbulence. Turbulence in the interstellar medium may be inhibited by gravity at large scales, and by self-gravity and EM forces at small scales, also producing fossils of previous active turbulence.

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