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Research
Origin and Evolution of Cosmic magnetic fields
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Image of rotation measure variance on
an angular scale of 1 degree (contours; top panel), constructed
from the catalog of rotation measures made from the NVSS (Taylor,
Stil & Sunstrum (2009). Note how RM avriance changes varies with
longitude and latitude, and mimics some well-known nearby
structures visible in the colour-coded H-alpha image in the background.
The bottom panel shows the slope of the second-order structure function of
rotation measure. From: Stil, Taylor & Sunstrum (2011)
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Integrated polarization of Galaxies (Stil, Krause, Beck & Taylor 2009).
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VLA Galactic Plane Survey (VGPS) (Stil, et al. 2006).
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Compact HI clouds with large forbidden velocities (Stil et al. 2006).
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