Instabilities near freshwater’s density maximum
his image by Laura Chandler and Marek Stastna (University of Waterloo) shows the instabilities that occur when a domain is initialized with 1C water above 8C water. This visualization was
CategoryVisualization
Stratospheric ozone intrusion
his animation by Alex Lupu (Environment and Climate Change Canada) and collaborators shows how stratospheric ozone can be transported into the troposphere during tropopause folding events and occasionally reach the
Turbulent wake behind a square block
his simulation and visualization by Zixiang Chen and Robert Martinuzzi (University of Calgary) shows the vorticity magnitude of the turbulent wake behind a square block mounted on a flat surface.
Shoaling internal solitary waves of elevation
This visualization of internal solitary waves was developed by Chengzhu Xu and Marek Stastna (Univ. Of Waterloo). These waves are commonly observed in the Earth’s atmosphere and oceans, e.g., large-amplitude
Simulations of lung surfactant
his animation by Svetlana Baoukina, Dmitri Rozmanov and Peter Tieleman (University of Calgary) shows a lipid monolayer in equilibrium with lipid vesicles on water surface. The lipids in vesicles and
Platinum-water interface
hese visualizations were developed by Kevin Ryczko and Isaac Tamblyn (UOIT). The platinum-water interface is of great interest in the field of electrochemistry. Platinum is known to be one of
Extreme nonlinear dynamics in light-driven nanoplasmas
irst-principle N-body simulations by Charles Varin (University of Ottawa) and collaborators with the HPC simulation engine MicPIC reveal the extreme dynamics of a nanoplasma driven by intense femtosecond infrared radiation.
Light-opals interaction in a 3D simulation
his animation by Antonino Calà Lesina and collaborators shows the interaction of a plane-wave optical pulse with a face-centered cubic photonic crystal (opals), formed by a lattice of polystyrene spheres
Dwarf Galaxy with SPH
his animation by David Williamson, Hugo Martel and Daisuke Kawata shows a single frame of a dwarf galaxy simulated with the SPH code GCD+ (written by Daisuke Kawata). The visualization
Ice/water system during ice melting
hese animations by Dmitri Rozmanov and Peter Kusalik (University of Calgary) demonstrate how discrete atoms and molecules can be visualized with a continuous 3D renderer, in this case ParaView.
Astrophysical Visualization with Custom Scripts and yt
n these examples a diffuse part of the astrophysical radiative transfer code FTTE (fully threaded transport engine) was adapted to do ray tracing at an arbitrary angle through a volume
Visualization of Mixed (Particles + 3D) Data with ParaView
ecently we worked with Alena Antipova and Colin Denniston from the Department of Applied Mathematics at Western University to visualize a numerical simulation of the motion of a nickel nanodisk
MAX3D: Visualization of X-ray Diffraction Patterns in 3D
AX3D is an interactive tool designed to read a series of 2D diffraction images and provide a visualization of a solid volume of reciprocal space (the Fourier space of a
SPH visualization with volume rendering
[su_vimeo url=”https://vimeo.com/135005892″ width=”100%”] his animation shows volume rendering of an SPH (smooth particle hydrodynamics) simulation of galaxy formation by Fabrice Durier (UVic) contaning 12 million particles, with dataset coloured by the