Supercomputing and E-Science Visualisation


DM->GAS->STARS->HTSMock rotation of LG64 M31 candidate

Simulation: Box=64Mpc/h, eff-resolution=4096^3

Redshift: ~0.9

Color coding: stars HST mock image- UVB=>RGB

Rendering region: R1~512kpc/h, R2~64kpc/h

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Gas distribution in Local group, CLUES B64_WM3

The image/movie shows the distribution of gas in the CLUES simulation B64_WM3_186592, a resimulation with 40963 particles, rendered with PMViewer. Colors represent the density of gas, from dark blue for sparse to bright yellow for very dense regions. The resimulated area was chosen because of its similarity to the Local Group, with Andromeda (M31) in the center, M33 to the lower right and the Milky Way at the upper right corner.

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Flight around Kepler2 targets

Flight around the 3D distribution of ~ 22,000 target stars for the Kepler2 mission. Each color corresponds to one K2 campaign, see NASA K2 webpage for more information and K2 fields for details on the observation campaigns. Stars from the original Kepler field are also shown, marked as grey points.
Campaign 9 is not included, since it points directly to the galactic center and no target stars were pre-selected.

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Random Playlist

Random Playlist

Example of a Random Playlist:


vlcplayer vis.m3u

Download: vis.m3u

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Orion nebula with MUSE

The MUSE spectrograph produces data cubes, consisting of image slices at different wave lengths. A number of such slices (fitted to characteristic emission lines) is shown in this movie. In the second part of the movie, only those slices are shown which make up the composite images (RGB) in the front. The wavelengths are given in nm.

Credits: Kristin Riebe, Peter Weilbacher, MUSE collaboration

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