Computational Astrophysics at the University of Minnesota
compastrouofm's Channel
 
Nat26 Color & Bmag compastro... - 3 views - 3 days ago
Similar to Nat17, but has background pressure perturbations mirroring magnetic perturbations
B ambient = 100
B jet = 10

Left-hand side is the color; Right-hand side is the magnetic field strength
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Nat19 Color compastro... - 6 views - 1 week ago
Nat19 JxB compastro... - 4 views - 1 week ago
Nat17 Bmag Movie compastro... - 21 views - 2 weeks ago
Time lapse simulation of Magnetic Field Strength of jet with beta = 10
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2-d Orszag-Tang Vortex compastro... - 27 views - 2 months ago
This is a 512x512 run of the standard MHD Orszag-Tang vortex test with the MHD-TVD solver. It runs for 1 dynamical time. The quantity imaged is density on a scale of 0.1 to 1. This simulation was done by Computational Astrophysics at the University of Minnesota Department of Astronomy. The simulation was done at the Minnesota Supercomputing Institute for Advanced Computational Research. The code is a new version of the MHD-TVD solver of Jones & Ryu, 1995 written by Peter Mendygral.
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TLS-F Model compastro... - 29 views - 6 months ago
This is a model of an non-inflated, buoyant, magnetized bubble moving through a tangled (on large scales), strong magnetic field in a galaxy cluster. The simulation was performed by Sean O'Neill of Computational Astrophysics at the University of Minnesota using the MHD-TVD code. Details of the calculation appear in O'Neill, De Young, & Jones (2009), available on astro-ph or in an April issue of The Astrophysical Journal.
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TLS Model compastro... - 14 views - 6 months ago
This is a model of an non-inflated, buoyant bubble moving through a tangled (on large scales), strong magnetic field in a galaxy cluster. The simulation was performed by Sean O'Neill of Computational Astrophysics at the University of Minnesota using the MHD-TVD code. Details of the calculation appear in O'Neill, De Young, & Jones (2009), available on astro-ph or in an April issue of The Astrophysical Journal.
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US-F Model compastro... - 16 views - 6 months ago
This is a model of an non-inflated, buoyant, magnetized bubble moving through a uniform, strong magnetic field in a galaxy cluster. The simulation was performed by Sean O'Neill of Computational Astrophysics at the University of Minnesota using the MHD-TVD code. Details of the calculation appear in O'Neill, De Young, & Jones (2009), available on astro-ph or in an April issue of The Astrophysical Journal.
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US Model compastro... - 22 views - 6 months ago
This is a model of an non-inflated, buoyant bubble moving through a uniform, strong magnetic field in a galaxy cluster. The simulation was performed by Sean O'Neill of Computational Astrophysics at the University of Minnesota using the MHD-TVD code. Details of the calculation appear in O'Neill, De Young, & Jones (2009), available on astro-ph or in an April issue of The Astrophysical Journal.
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TLS-I Model compastro... - 16 views - 6 months ago
This is a model of an inflated, buoyant bubble moving through a tangled (on large scales), strong magnetic field in a galaxy cluster. The simulation was performed by Sean O'Neill of Computational Astrophysics at the University of Minnesota using the MHD-TVD code. Details of the calculation appear in O'Neill, De Young, & Jones (2009), available on astro-ph or in an April issue of The Astrophysical Journal.
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TBS-I Model compastro... - 27 views - 6 months ago
This is a model of an inflated, buoyant bubble moving through a tangled (on bubble scales), strong magnetic field in a galaxy cluster. The simulation was performed by Sean O'Neill of Computational Astrophysics at the University of Minnesota using the MHD-TVD code. Details of the calculation appear in O'Neill, De Young, & Jones (2009), available on astro-ph or in an April issue of The Astrophysical Journal.
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US-I Model compastro... - 31 views - 6 months ago
This is a model of an inflated, buoyant bubble moving through a uniform, strong magnetic field in a galaxy cluster. The simulation was performed by Sean O'Neill of Computational Astrophysics at the University of Minnesota using the MHD-TVD code. Details of the calculation appear in O'Neill, De Young, & Jones (2009), available on astro-ph or in an April issue of The Astrophysical Journal.
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compastrouofm  
Profile
 
Channel Views:
191
Age:
27
Joined:
December 15, 2008
Last Sign In:
3 days ago
Videos Watched:
211
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Videos from the University of Minnesota Department of Astronomy's Computational Astrophysics Group.
About Me: Computational Astrophysics Group at University of Minnesota
Hometown:
Minneapolis
Country:
United States
Hobbies:
Astronomy and Astrophysics, Simulations, Numerical Methods
Recent Activity  
compastrouofm uploaded a new video (3 days ago)
Similar to Nat17, but has background pressure perturbations mirroring magnetic perturbations
B ambient = 100
B jet = 10

Left-hand side is the color; R...   more
 
 
compastrouofm became friends with umncla (1 week ago)
 
 
compastrouofm uploaded a new video (1 week ago)
 
 
compastrouofm uploaded a new video (1 week ago)
 
 
compastrouofm uploaded a new video (2 weeks ago)
Time lapse simulation of Magnetic Field Strength of jet with beta = 10
 
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