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Knowledge of the coronal magnetic field is crucial for assessing theories of coronal heating and origin of the solar wind. One of the few ways of measuring the magnetic field in the corona is via Faraday rotation of linearly polarized radio signals which have propagated through the corona and been
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1. Simultaneous VLA and UVCS/SOHO Observations of the Solar Corona Steven R. Spangler (University of Iowa), Mari Paz Miralles, Steven R. Cranmer, and John C. Raymond (Harvard-Smithsonian CFA)
3. Coronal Faraday Rotation
5. The corona on August 16, 2003
7. Measured Coronal Faraday Rotation
9. UVCS Measurements
11. Why was such a large Rotation Measure event observed?
14. Thanks