The theory of interstellar turbulence generation

Details The theory of interstellar turbulence generation The theory of interstellar turbulence generation

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..145b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, Feb. 1988, p. 145-150. In Russian. In Russian.

Statistics

Computation

2

Astronomical Models, Interstellar Matter, Magnetohydrodynamic Turbulence, Computational Astrophysics, Hydrodynamic Equations, Spectral Energy Distribution

Scientific paper

An hydrodynamical model for turbulence formation in a diffuse interstellar medium (ISM) is developed. Turbulence generation takes place due to interaction of hydrodynamical modes with an ensemble of shocks and due to nonlinear effects of spectral energy transfer. Fluctuation spectra for ISM parameters are derived and are shown to be fitted by power-law functions in various wave-number domains.

Affiliated with

Also associated with

No associations

Rating

The theory of interstellar turbulence generation does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The theory of interstellar turbulence generation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The theory of interstellar turbulence generation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1227889