VLBI measurements of interstellar turbulence spectra

Details VLBI measurements of interstellar turbulence spectra VLBI measurements of interstellar turbulence spectra

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aipc..174..122m&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

Astronomy and Astrophysics

Astronomy

5

Interstellar Matter, Magnetohydrodynamic Turbulence, Radio Scattering, Radio Sources (Astronomy), Very Long Base Interferometry, Cygnus Constellation, Quasars, Radio Interferometers, Wave Propagation

Scientific paper

VLBI observations of the scattered images of two compact radio sources whose lines of sight pass through the Cyg superbubble region were analyzed to infer the spatial spectrum of intervening turbulence. For the quasar 2005 + 403, the phase structure function varies quadratically with projected baseline for b less than 4 x 10 to the 8th cm, but then flattens to a slope near zero. This is inconsistent with type B power-law turbulence unless the outer scale is 2 x 10 to the 9th cm.

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