  We present an extension of the Coronal Reconstruction Onto B-Aligned Regions
(CROBAR) method to Linear Force Free Field (LFFF) extrapolations, and apply it
to the reconstruction of a set of AIA, MDI, and STEREO EUVI data. The results
demonstrate that CROBAR can not only reconstruct coronal emission structures,
but also that it can help constrain the coronal field extrapolations via the
LFFF's helicity $\alpha$ parameter. They also provide a real-world example of
how CROBAR can easily incorporate information from multiple perspectives to
improve its reconstructions, and we also use the additional perspectives to
help validate the reconstructions. We furthermore touch on the use of
real-world emission passbands rather than idealized power-law type ones using
DEMs. We conclude with a comparison of CROBAR generated emission to observed
emission and those produced with idealized DEM based power-laws. These results
further illustrate the promise of CROBAR for real-world applications, and we
make available a preliminary release of the software available for download.

Solar and Stellar Astrophysics