  We describe a new technique to measure the height of the X-ray limb with
observations from occulted X-ray flare sources as observed by the RHESSI (the
Reuven Ramaty High-Energy Spectroscopic Imager) satellite. This method has
model dependencies different from those present in traditional observations at
optical wavelengths, which depend upon detailed modeling involving radiative
transfer in a medium with complicated geometry and flows. It thus provides an
independent and more rigorous measurement of the "true" solar radius, meaning
that of the mass distribution. RHESSI's measurement makes use of the flare
X-ray source's spatial Fourier components (the visibilities), which are
sensitive to the presence of the sharp edge at the lower boundary of the
occulted source. We have found a suitable flare event for analysis,
SOL2011-10-20T03:25 (M1.7), and report a first result from this novel technique
here. Using a 4-minute integration over the 3-25 keV photon energy range, we
find $R_{\mathrm{X-ray}} = 960.11\ \pm\ 0.15 \pm 0.29$ arcsec, at 1 AU, where
the uncertainties include statistical uncertainties from the method and a
systematic error. The standard VAL-C model predicts a value of 959.94 arcsec,
about 1$\sigma$ below our value.
