Changes between Version 183 and Version 184 of u/madams/CollidingFlowsFigures


Ignore:
Timestamp:
02/19/15 16:03:47 (10 years ago)
Author:
madams
Comment:

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  • u/madams/CollidingFlowsFigures

    v183 v184  
    3232[[br]]The gray scale is for the thermal pressure vs density plots, and the color scale is the magnetic pressure vs. density plots. The line is T=10K, dotted line = ram pressure of the flows, and dashed line = initial magnetic pressure.
    3333
    34 [[Image(S0_BvnFigure-new.png, width=800)]]
     34[[Image(S0BvnFigure.png, width=800)]]
    3535
    3636'''[https://astrobear.pas.rochester.edu/trac/wiki/u/erica/CF_spectra Spectra]''' [[br]] Gravitational energy spectra made by taking the Fourier Transform of Sqrt(-gravitational_energy) to avoid nans, since the gravitational energy was everywhere negative.
    … …  
    8989'''[https://astrobear.pas.rochester.edu/trac/wiki/u/erica/CF_bvn_plot B vs. n]'''[[br]]The gray scale is for the thermal pressure vs density plots, and the color scale is the magnetic pressure vs. density plots. The line is T=10K, dotted line = ram pressure of the flows, and dashed line = initial magnetic pressure.
    9090
    91 [[Image(S15_BvnFigure-new.png, width=800)]]
     91[[Image(S15BvnFigure.png, width=800)]]
    9292
    9393'''[https://astrobear.pas.rochester.edu/trac/wiki/u/erica/CF_spectra Spectra]''' [[br]] Gravitational energy spectra made by taking the Fourier Transform of Sqrt(-gravitational_energy) to avoid nans, since the gravitational energy was everywhere negative.
    … …  
    118118'''[https://astrobear.pas.rochester.edu/trac/wiki/u/erica/CF_bvn_plot B vs. n]'''[[br]]The gray scale is for the thermal pressure vs density plots, and the color scale is the magnetic pressure vs. density plots. The line is T=10K, dotted line = ram pressure of the flows, and dashed line = initial magnetic pressure.
    119119
    120 [[Image(S30_BvnFigure-new.png, width=800)]]
     120[[Image(S30BvnFigure.png, width=800)]]
    121121
    122122
    … …  
    148148'''[https://astrobear.pas.rochester.edu/trac/wiki/u/erica/CF_bvn_plot B vs. n]'''[[br]]The gray scale is for the thermal pressure vs density plots, and the color scale is the magnetic pressure vs. density plots. The line is T=10K, dotted line = ram pressure of the flows, and dashed line = initial magnetic pressure.
    149149
    150 [[Image(S60_BvnFigure-new.png, width=800)]]
     150[[Image(S60BvnFigure.png, width=800)]]
    151151
    152152'''[https://astrobear.pas.rochester.edu/trac/wiki/u/erica/CF_spectra Spectra]''' [[br]] Gravitational energy spectra made by taking the Fourier Transform of Sqrt(-gravitational_energy) to avoid nans, since the gravitational energy was everywhere negative.
    … …  
    229229[[CollapsibleStart(B vs. n)]]The gray scale is for the thermal pressure vs density plots, and the color scale is the magnetic pressure vs. density plots. The line is T=10K, dotted line = ram pressure of the flows, and dashed line = initial magnetic pressure.
    230230
    231 || '''Shear 0''' || [[Image(S0_BvnFigure-new.png, width=800)]] ||
    232 || '''Shear 15''' || [[Image(S15_BvnFigure-new.png, width=800)]] ||
    233 || '''Shear 30''' || [[Image(S30_BvnFigure-new.png, width=800)]] ||
    234 || '''Shear 60''' || [[Image(S60_BvnFigure-new.png, width=1050)]] ||
     231|| '''Shear 0''' || [[Image(S0BvnFigure.png, width=800)]] ||
     232|| '''Shear 15''' || [[Image(S15BvnFigure.png, width=800)]] ||
     233|| '''Shear 30''' || [[Image(S30BvnFigure.png, width=800)]] ||
     234|| '''Shear 60''' || [[Image(S60BvnFigure.png, width=1050)]] ||
    235235[[CollapsibleEnd]]
    236236