Magnetic Turbulence in the WIM

Details Magnetic Turbulence in the WIM Magnetic Turbulence in the WIM

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004assl..315..295m&link_type=abstract

How Does the Galaxy Work? A Galactic Tertulia with Don Cox and Ron Reynolds. Edited by Emilio J. Alfaro, Instituto de Astrofica

Astronomy and Astrophysics

Astrophysics

Scientific paper

The turbulence in the Galactic magnetic field can be measured using Faraday rotation measures towards extra-galactic radio sources along with Hα emission measures from the Warm Ionized Medium in our galaxy. This has now been done for two 10° by 10° regions of the sky centered on (l,b)=145°, -20° (Minter & Spangler 1996), and 185°, +20°. I will present preliminary results for the 185°,+20° region.

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