VIVID
3D Visualization and animation tool, by Naftali Deustch
We present VIVID, an innovative method for research using 3D technology.
Alongside theoretical and experimental studies, one of the useful tools for research in the field of physics is the numerical simulation. Powerful as it is, the understanding of simulation may be difficult. The typical way to visually inspect the simulations, 2D projections, allows the researcher to develop intuition and understanding of the simulation. However, not all the details of a given simulation are visible in such a plot. We find that involving 3D tools in scientific research can be profitable, and given the interactive nature of 3D, it can fill the gaps left by the 2D projections. The following developed tool enables new points of view for researchers and facilitates discoveries.
VIVID uses a Voronoi code package to represent the simulated data as polygons. The tool proceeds to clear the data resulting in a surface. Later using algorithms of Smooth, decimation and Double Points handling it sharpens the model features, resulting in a clear, easy to study model. By presenting the simulation as fully interactive 3D models, we can make the process of analyzing the simulation faster and efficient, enabling visualizing hidden by 2D physical dynamics — the creation of such models is done in VIVID by just one simple line of code.
VIVID was tested in our cosmology research group by producing models from simulations for researchers, supporting new scientific insights about the evolution of galaxies and structures of the Universe.
Models
Filament and galaxy formation within it - surfaces are gas densities. 10^-24 [gr/cm^3] - yellow 10^-25 [gr/cm^3] - blue 10^-26 [gr/cm^3] - purple. Box size of 140 [kpc].
We can see the easy navigation and sharing of models, in which we can observe features of the filament as the distance between galaxies, shapes of gas and general structure is now visible to understand and find new study ideas.
Galaxy disk structure and clump structures - the surface is gas density 10^-24 [gr/cm^3].
Galaxy and halo gas corona - color describes temperature from cold (purple) to hot (red), surfaces are 10^-24, 10^-25, 10^-26 and 10^-27 gr/cm^3.
We can see in this example a structure in the gas corona.
Satellite galaxy evolution - surfaces are gas densities. 10^-24 [gr/cm^3] - yellow 10^-25 [gr/cm^3] - pink 10^-26 [gr/cm^3]. We can see the gas dynamics inside the halo (further details in the soon to be published paper).
Satellite stellar evolution - tidal stripping in the halo. (in yellow, the stellar component)
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