Michael Thompson & Dr. Huei-Ping School for Engineering of Matter, Transport, and Energy A Classroom Model for Understanding Earth’s Climate Change Background: This project uses a rotating tank to conduct fluid experiments for studying the sensitivity of Earth’s climate to external perturbations.
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Contours of tangential velocity of the tank in CFD solver ANSYS-Fluent of the experimental rotational fluid tank in Paraview/Matlab.
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Temperature Profile of the experimental rotational fluid tank in Paraview/Matlab.
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Michael Thompson School for Engineering of Matter, Transport, and Energy A Computational Study of Transient Couette Flow Over an Embedded Cavity Surface How aerodynamic efficient are Butterflies flexible, micro-geometrically surface patterned, scaled wings? The above picture is a comparison of Inclined Scales.
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Dr. Marcus Herrmann Atomization of a liquid jet in crossflow.
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Dr. Marcus Herrmann Atomization of a liquid jet in crossflow.
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Dr. Marcus Herrmann Breakup of a Diesel jet injected into a high pressure environment.
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Upstream view of the atomization of a liquid jet injected into a crossflow.
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From Left to Right: A time averaged view of a turbulent jet flame, a high speed image of a turbulent jet flame, and a high speed image of a bluff body stabilized turbulent flame.
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Will Gray 2-D snapshots showing (from left to right) the density, temperature, amount of H2, and amount of metals during the initial impact from the shock.
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2-D snapshots shows (from left to right) the density, temperature, amount of H2, and amount of metals during the collapse of the gas cloud.
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Panel of images showing the evolution of a shock overtaking a gas cloud from initially separate (top left) to surrounding and compressing the gas (top right and bottom left) and the final state of the gas (bottom right).
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Dr. Andrew Bordner Mayo Clinic Backbone structures for three different peptides after 50 ns all-atom molecular dynamics simulations with explicit solvent. The three darker colors show three different peptides bound to their protein receptors, while the three lighter colors show the peptides unbound in a solution.
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Patrick Young, ASU. These images show the density of material in an expanding Supernova approximately one year after the explosion. Two kinds of structures are seen in the images: structures generated by instabilities by the passing of the blast's shock wave, and those structures caused by the expansion of material being heated by the radioactive decay nickel (the inner, brighter structures). The structures formed in the explosion are important to the delivery of newly synthesized chemical elements. This image depicts the spherical explosion.
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Image showing explosion vs degree of bipolar asymmetry.
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Image showing explosion with different degrees of bipolar asymmetry.
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C. Michael Gilbert . Molecular dynamics simulation of a hypothetical gigahertz oscillator made from two carbon nanotubes. Work carried out as part of the final project in ASU Physics course PHY494/PHY598 (Spring 2012, instructor Dr Oliver Beckstein). Simulations were performed on saguaro at A2C2.
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Dr. Liubin Pan . Three-dimensional renderings of a clump of supernova material fragmenting as it enters a cloud of gas. Colors indicate the density, and three clumps of different sizes are shown. Larger clumps are seen to fragment more.
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credit: Melissa Morris, school of earth and space exploration. The image shows a bow shock around a planetary embryo the size of a proto-Mars.
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