Anisotropic Turbulence in the Interstellar Medium Towards W49N

Details Anisotropic Turbulence in the Interstellar Medium Towards W49N Anisotropic Turbulence in the Interstellar Medium Towards W49N

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aas...187.4505d&link_type=abstract

American Astronomical Society, 187th AAS Meeting, #45.05; Bulletin of the American Astronomical Society, Vol. 27, p.1348

Astronomy and Astrophysics

Astronomy

Scientific paper

Interstellar turbulence produces fluctations of electron density over more than seven decades of spatial scales in the interstellar medium. Diffraction of radio-waves around these density fluctuations causes an increase in the observed angular sizes of compact radio sources. Measurements of this angular broadening can, in principle, completely characterize interstellar turbulence on all spatial scales. We present here measurements of parameters of the anisotropic turbulence seen towards W49N.

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