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We have undertaken a major enhancement of our IDL-based simulation toolsdeveloped earlier for modeling microwave and X-ray emission. The object-basedarchitecture provides an interactive graphical user interface that allows theuser to import photospheric magnetic field maps and perform magnetic fieldextrapolations to almost instantly generate 3D magnetic field models, toinvestigate the magnetic topology of these models by interactively creatingmagnetic field lines and associated magnetic flux tubes, to populate the fluxtubes with user-defined nonuniform thermal plasma and anisotropic, nonuniform,nonthermal electron distributions; to investigate the spatial and spectralproperties of radio and X-ray emission calculated from the model, and tocompare the model-derived images and spectra with observational data. Theapplication integrates shared-object libraries containing fast gyrosynchrotronemission codes developed in FORTRAN and C++, soft and hard X-ray codesdeveloped in IDL, a FORTRAN-based potential-field extrapolation routine and anIDL-based linear force free field extrapolation routine. The interactiveinterface allows users to add any user-defined radiation code that adheres toour interface standards, as well as user-defined magnetic field extrapolationroutines. Here we use this tool to analyze a simple single-loop flare and usethe model to constrain the 3D structure of the magnetic flaring loop and 3Dspatial distribution of the fast electrons inside this loop. We iterativelycompute multi-frequency microwave and multi-energy X-ray images from realisticmagnetic fluxtubes obtained from an extrapolation of a magnetogram taken priorto the flare, and compare them with imaging data obtained by SDO, NoRH, andRHESSI instruments. We use this event to illustrate use of the tool for generalinterpretation of solar flares to address disparate problems in solar physics.

3D Radio and X-Ray Modeling and Data Analysis Software: Revealing Flare Complexity