The nature of interstellar turbulence

Details The nature of interstellar turbulence The nature of interstellar turbulence

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981azh....58..534a&link_type=abstract

Astronomicheskii Zhurnal, vol. 58, May-June 1981, p. 534-541. In Russian.

Astronomy and Astrophysics

Astronomy

1

Cosmic Plasma, Interstellar Gas, Plasma Turbulence, Radio Sources (Astronomy), Shock Wave Propagation, Stellar Winds, B Stars, Electron Density (Concentration), Hydrogen Clouds, Magnetohydrodynamic Flow, O Stars, Plasma Density, Plasma Waves, Pulsars, Scintillation, X Ray Sources

Scientific paper

Factors determining the formation of the interstellar scintillation pattern of discrete radio sources are examined. It is shown that one of the factors is magnetoacoustic turbulence, which arises as a result of shock wave propagation at a velocity of 20-100 km/s in the interstellar medium and also as a result of the inhomogeneity of stellar wind from OB stars.

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