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

High-fidelity 3D Reconstruction of Solar Coronal Physics with the Updated CROBAR Method