REFERENCES PERTAINING TO SOLAR CORONAL MAGNETIC FIELDS:

(1) "Radio Measurements of the Height of Strong Coronal Magnetic Fields Above
Sunspots at the Solar Limb," J. W. Brosius and S. M. White, ApJ 641, L69 (2006 April 10).
http://www.journals.uchicago.edu/ApJ/journal/issues/ApJL/v641n1/20411/20411.html

(2) "Close Association of an Extreme-Ultraviolet Sunspot Plume with
Depressions in the Sunspot Radio Emission," J. W. Brosius and S. M.
White, ApJ 601, 546 (2004 January 20).
http://www.journals.uchicago.edu/ApJ/journal/issues/ApJ/v601n1/58729/58729.html

(3) "Coronal Diagnostics with Coordinated Radio and EUV/Soft X-Ray
Observations," J. W. Brosius, in "Solar and Space Weather Radiophysics,"
eds. D. E. Gary and C. O. Keller (Dordrecht: Kluwer), p. 265 (2004).

(4) "Measurements of Three-Dimensional Coronal Magnetic Fields from
Coordinated Extreme-Ultraviolet and Radio Observations of a Solar
Active Region Sunspot," J. W. Brosius, E. Landi, J. W. Cook, J. S.
Newmark, N. Gopalswamy, and A. Lara, ApJ 574, 453 (2002 July 20).
http://www.journals.uchicago.edu/ApJ/journal/issues/ApJ/v574n1/54833/54833.html

(5) "Coronal Magnetography of a Solar Active Region Using Coordinated
SERTS and VLA Observations," J. W. Brosius, J. M. Davila, R. J.
Thomas, and S. M. White, ApJ 488, 488 (1997 October 10).
http://www.journals.uchicago.edu/ApJ/journal/issues/ApJ/v488n1/35624/35624.html