Probing the Large Scale Plasma Structure of the Solar Corona with Faraday Rotation Measurements

Details Probing the Large Scale Plasma Structure of the Solar Corona with Faraday Rotation Measurements Probing the Large Scale Plasma Structure of the Solar Corona with Faraday Rotation Measurements

2007-01-18

arxiv.org/abs/astro-ph/0701538v1

Astrophys.J.668:520-532,2007

Astronomy and Astrophysics

Astrophysics

32 pages, 7 figures

Scientific paper

10.1086/521140

Faraday rotation measurements of the solar corona made with the Very Large Array (VLA) at frequencies of 1465 and 1665 MHz are reported. The measurements were made along 20 lines of sight to 19 extragalactic radio sources in March and April, 2005. The closest heliocentric distances of the lines of sight ranged from 9.7 to 5.6 $R_{\odot}$. Measured rotation measures range from -25 to +61 rad/m$^2$. The purpose of these observations is to probe the three dimensional structure of the coronal plasma in the heliocentric distance range $5-10 R_{\odot}$, and particularly the strength and structure of the coronal magnetic field. The measured rotation measures are compared with models for the coronal plasma structure. For the majority of the lines of sight, the observed rotation measures are reasonably well represented by the predictions from the models. However, 4 of the 20 lines of sight have large observed-model residuals, which do not seem associated with coronal mass ejections. The magnitude of the field necessary to reproduce the majority of the observations is in the range 46-120 milliGauss at $5 R_{\odot}$, with a smaller, preferred range of 46-52 mG at $5 R_{\odot}$.

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