Changes between Version 168 and Version 169 of u/madams/CollidingFlowsFigures


Ignore:
Timestamp:
02/06/15 16:33:39 (10 years ago)
Author:
madams
Comment:

—

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  • u/madams/CollidingFlowsFigures

    v168 v169  
    3030[[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.
    3131
    32 [[Image(S0_BvnFigure.png, 90%)]]
     32[[Image(S0_BvnFigure.png, width=800)]]
    3333
    3434'''[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.
    3535
    3636|| ''Time Evolution View'' || ''Energy Evolution View'' ||
    37 || [[Image(s0_spectra_brick_tevol.png, 75%)]] || [[Image(s0_energyspectra_brick_eevol.png, 75%)]] ||
     37|| [[Image(s0_spectra_brick_tevol.png, width=400)]] || [[Image(s0_energyspectra_brick_eevol.png, width=400)]] ||
    3838
    3939
    … …  
    4242 
    4343
    44 [[Image(E1.png, 35%)]][[br]]This plot shows each of the energies (grav., mag., kinetic), divided by the initial kinetic energy in the collision region. It shows that the dominant energy in the collision region is kinetic.
    45 
    46 
    47 
    48 [[Image(E2.png, 35%)]][[br]]This plot shows each of the energies (grav., mag., kinetic), divided by their own initial values, showing how much each of the energies change over time. It shows that the gravitational energy has the steepest growth rate of these 3 energies. The curve reaches a peak plateau at about 10 Myr, coinciding with the formation of the first sink.
    49 
    50 
    51 [[Image(E3.png, 35%)]][[br]]This plot shows each of the energies (grav., mag.), divided by the kinetic energy at each time; it is an instantaneous view of the ratio of these energies to the kinetic energy in the collision region. It shows that after the steep growth in gravitational energy (after 10 Myr), the gravitational energy remains only at about 25% the kinetic. The magnetic energy remains a much smaller fraction throughout the simulation.
     44[[Image(E1.png, width=400)]][[br]]This plot shows each of the energies (grav., mag., kinetic), divided by the initial kinetic energy in the collision region. It shows that the dominant energy in the collision region is kinetic.
     45
     46
     47
     48[[Image(E2.png, width=400)]][[br]]This plot shows each of the energies (grav., mag., kinetic), divided by their own initial values, showing how much each of the energies change over time. It shows that the gravitational energy has the steepest growth rate of these 3 energies. The curve reaches a peak plateau at about 10 Myr, coinciding with the formation of the first sink.
     49
     50
     51[[Image(E3.png, width=400)]][[br]]This plot shows each of the energies (grav., mag.), divided by the kinetic energy at each time; it is an instantaneous view of the ratio of these energies to the kinetic energy in the collision region. It shows that after the steep growth in gravitational energy (after 10 Myr), the gravitational energy remains only at about 25% the kinetic. The magnetic energy remains a much smaller fraction throughout the simulation.
    5252
    5353'''Streamline Plots (Global vs. local views)''' [[br]] Some example streamline plots
    5454
    5555{{{#!comment
    56 [[Image(streams.png, 60%)]][[br]]
     56[[Image(streams.png, width=400)]][[br]]
    5757}}}
    58 [[Image(sweetness0002.png, 60%)]][[br]]
    59 [[Image(streamlines_CF2.png, 30%)]][[br]]
     58[[Image(sweetness0002.png, width=400)]][[br]]
     59[[Image(streamlines_CF2.png, width=400)]][[br]]
    6060
    6161'''Down y-axis global view''' [[br]]
    62 [[Image(globalblk_S0_downy0001.png, 40%)]]
     62[[Image(globalblk_S0_downy0001.png, width=400)]]
    6363
    6464'''Streamline Global View''' [[br]]
    65 || [[Image(globalblk_S00001.png, 90%)]] || [[Image(globalblk_S0_downbarrel0001.png, 90%)]] ||
     65|| [[Image(globalblk_S00001.png, width=400)]] || [[Image(globalblk_S0_downbarrel0001.png, width=400)]] ||
    6666[[CollapsibleEnd]]
    6767
    … …  
    7272'''[https://astrobear.pas.rochester.edu/trac/wiki/u/erica/CF_coldens Column Density Map] with Sinks (left) & [https://astrobear.pas.rochester.edu/trac/wiki/u/erica/CF_BetaMaps Inverse Beta Maps] (right)'''
    7373
    74 || [[Image(s15cdm-02062015.png)]] || [[Image(s15invbeta-02062015.png)]] ||
     74|| [[Image(s15cdm-02062015.png, width=400)]] || [[Image(s15invbeta-02062015.png, width=400)]] ||
    7575
    7676'''Sink Notes:'''
    … …  
    8787'''[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.
    8888
    89 [[Image(S15_BvnFigure.png, 90%)]]
     89[[Image(S15_BvnFigure.png, width=800)]]
    9090
    9191'''[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.
    9292
    9393|| ''Time Evolution View'' || ''Energy Evolution View'' ||
    94 || [[Image(s15_spectra_brick_tevol.png, 75%)]] || [[Image(s15_energyspectra_brick_eevol.png, 75%)]] ||
     94|| [[Image(s15_spectra_brick_tevol.png, width=400)]] || [[Image(s15_energyspectra_brick_eevol.png, width=400)]] ||
    9595
    9696'''Streamline Global View''' [[br]]
    97 || [[Image(globalblk_S150000.png, 90%)]] || [[Image(globalblk_S15_tilted0000.png, 90%)]] || [[Image(globalblk_S15_downbarrel0000.png, 90%)]] ||
     97|| [[Image(globalblk_S150000.png, width=400)]] || [[Image(globalblk_S15_tilted0000.png, width=400)]] || [[Image(globalblk_S15_downbarrel0000.png, width=400)]] ||
    9898
    9999[[CollapsibleEnd]]
    … …  
    105105'''[https://astrobear.pas.rochester.edu/trac/wiki/u/erica/CF_coldens Column Density Map] with Sinks (left) & [https://astrobear.pas.rochester.edu/trac/wiki/u/erica/CF_BetaMaps Inverse Beta Maps] (right)'''
    106106
    107 || [[Image(s30cdm-02062015.png)]] || [[Image(s30invbeta-02062015.png)]] ||
     107|| [[Image(s30cdm-02062015.png, width=400)]] || [[Image(s30invbeta-02062015.png, width=400)]] ||
    108108
    109109'''Sink Notes:'''
    … …  
    116116'''[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.
    117117
    118 [[Image(S30_BvnFigure.png, 90%)]]
     118[[Image(S30_BvnFigure.png, width=800)]]
    119119
    120120
    … …  
    122122
    123123|| ''Time Evolution View'' || ''Energy Evolution View'' ||
    124 || [[Image(s30_spectra_brick_tevol.png, 75%)]] || [[Image(s30_energyspectra_brick_eevol.png, 75%)]] ||
     124|| [[Image(s30_spectra_brick_tevol.png, width=400)]] || [[Image(s30_energyspectra_brick_eevol.png, width=400)]] ||
    125125
    126126'''Streamline Global View''' [[br]]
    127 || [[Image(globalblk_S300000.png, 50%)]] || [[Image(globalblk_S30_tilted0001.png, 90%)]] || [[Image(globalblk_S30_downbarrel0002.png, 90%)]] ||
     127|| [[Image(globalblk_S300000.png, width=400)]] || [[Image(globalblk_S30_tilted0001.png, width=400)]] || [[Image(globalblk_S30_downbarrel0002.png, width=400)]] ||
    128128
    129129[[CollapsibleEnd]]
    … …  
    135135'''[https://astrobear.pas.rochester.edu/trac/wiki/u/erica/CF_coldens Column Density Map] with Sinks (left) & [https://astrobear.pas.rochester.edu/trac/wiki/u/erica/CF_BetaMaps Inverse Beta Maps] (right)'''
    136136
    137 || [[Image(s60cdm-02062015.png)]] || [[Image(s60invbeta-02062015.png)]] ||
     137|| [[Image(s60cdm-02062015.png, width=400)]] || [[Image(s60invbeta-02062015.png, width=400)]] ||
    138138
    139139'''Sink Notes:'''
    … …  
    146146'''[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.
    147147
    148 [[Image(S60_BvnFigure.png, 90%)]]
     148[[Image(S60_BvnFigure.png, width=800)]]
    149149
    150150'''[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.
    151151
    152152|| ''Time Evolution View'' || ''Energy Evolution View'' ||
    153 || [[Image(s60_spectra_brick_tevol.png, 75%)]] || [[Image(s60_energyspectra_brick_eevol.png, 75%)]] [[Image(s60_33myr_energies.png, 40%)]] ||
     153|| [[Image(s60_spectra_brick_tevol.png, width=400)]] || [[Image(s60_energyspectra_brick_eevol.png, width=400)]] [[Image(s60_33myr_energies.png, width=400)]] ||
    154154
    155155'''Streamlines Global View''' [[br]]
    156156
    157 || [[Image(globalblk_S600000.png, 90%)]] || [[Image(globalblk_S60_tilted0001.png, 90%)]] || [[Image(globalblk_S60_downbarrel0000.png, 90%)]] ||
     157|| [[Image(globalblk_S600000.png, width=400)]] || [[Image(globalblk_S60_tilted0001.png, width=400)]] || [[Image(globalblk_S60_downbarrel0000.png, width=400)]] ||
    158158
    159159[[CollapsibleEnd]]
    … …  
    201201== Charts ==
    202202
    203 || [[Image(sinkschart_1.png, width=500)]] [[br]] '''Figure 1.''' The blue & right hand vertical axis indicates the total mass in solar masses (i.e. summation of all the masses) of the sinks in that particular run series by the final frame. The red & right hand vertical axis measures the number of sinks that formed in total for that run series. Note that Shear 60 is the only run that did not form a sink before 27.3 Myr (rather 32.8 Myr). || [[Image(bamfgraph.png, width=500)]] [[br]] '''Figure 2.''' The individual masses and formation times of the cores formed for each run series as denoted by the different colors. The sinks are numbered and colored by order of formation. One can see that they add up to the total mass illustrated in Figure 1. || [[Image(SinkBins_diff.png, width=500)]] [[br]] '''Figure 3.''' A column chart that indicates the number of sinks that form that are binned for 0-10, 10-100, and 100-1000 solar masses for each run. The runs are illustrated by color. ||
    204 
     203|| [[Image(sinkschart_1.png, width=400)]] [[br]] '''Figure 1.''' The blue & right hand vertical axis indicates the total mass in solar masses (i.e. summation of all the masses) of the sinks in that particular run series by the final frame. The red & right hand vertical axis measures the number of sinks that formed in total for that run series. Note that Shear 60 is the only run that did not form a sink before 27.3 Myr (rather 32.8 Myr). || [[Image(bamfgraph.png, width=400)]] [[br]] '''Figure 2.''' The individual masses and formation times of the cores formed for each run series as denoted by the different colors. The sinks are numbered and colored by order of formation. One can see that they add up to the total mass illustrated in Figure 1. || [[Image(SinkBins_diff.png, width=400)]] [[br]] '''Figure 3.''' A column chart that indicates the number of sinks that form that are binned for 0-10, 10-100, and 100-1000 solar masses for each run. The runs are illustrated by color. ||
    205204[[CollapsibleEnd]]
    206205
    … …  
    208207
    209208[[CollapsibleStart(Spectra Table: Energies vs. Time)]]
    210 
    211 [[Image(energies_vs_time_bricolette.png, 75%)]]
    212 
     209[[Image(energies_vs_time_bricolette.png, width=1000)]]
    213210{{{#!comment
    214211|| '''Time-Energy''' || '''Gravitational''' || '''Magnetic''' || '''Kinetic''' ||
    215 || '''0 Myr''' || [[Image(grav_0frame0000.png, 90%)]] || [[Image(mag_0frame0000.png, 90%)]] || [[Image(kin_0frame0000.png, 90%)]] ||
    216 || '''10 Myr''' || [[Image(grav_101frame0000.png, 90%)]] || [[Image(mag_101frame0000.png, 90%)]] || [[Image(kin_101frame0000.png, 90%)]] ||
    217 || '''20 Myr''' || [[Image(grav_202frame0000.png, 90%)]] || [[Image(mag_202frame0000.png, 90%)]] || [[Image(kin_202frame0000.png, 90%)]] ||
    218 || '''27 Myr''' || [[Image(grav_273frame0000.png, 90%)]] || [[Image(mag_273frame0000.png, 90%)]] || [[Image(kin_273frame0000.png, 90%)]] ||
     212|| '''0 Myr''' || [[Image(grav_0frame0000.png, width=400)]] || [[Image(mag_0frame0000.png, width=400)]] || [[Image(kin_0frame0000.png, width=400)]] ||
     213|| '''10 Myr''' || [[Image(grav_101frame0000.png, width=400)]] || [[Image(mag_101frame0000.png, width=400)]] || [[Image(kin_101frame0000.png, width=400)]] ||
     214|| '''20 Myr''' || [[Image(grav_202frame0000.png, width=400)]] || [[Image(mag_202frame0000.png, width=400)]] || [[Image(kin_202frame0000.png, width=400)]] ||
     215|| '''27 Myr''' || [[Image(grav_273frame0000.png, width=400)]] || [[Image(mag_273frame0000.png, width=400)]] || [[Image(kin_273frame0000.png, width=400)]] ||
    219216}}}
    220 
    221217[[CollapsibleEnd]]
    222218
    … …  
    225221Legend: [[br]] '''srho_vx_total''' = kinetic energy, '''sBx_Field_total''' = magnetic energy, '''SqrtGravEnergy_Field''' = gravitational energy
    226222}}}
    227 
    228 [[Image(energyspectra_vs_time_brickeronie.png, 75%)]]
    229 
     223[[Image(energyspectra_vs_time_brickeronie.png, width=1000)]]
    230224{{{#!comment
    231225|| '''Time-Run''' || '''Shear 0''' || '''Shear 15''' || '''Shear 30''' || '''Shear 60''' ||
    232 || '''0 Myr''' || [[Image(s0_0myr0000.png, 90%)]] || [[Image(s15_0myr0000.png, 90%)]] || [[Image(s30_0myr0000.png, 90%)]] || [[Image(s60_0myr0000.png, 90%)]] ||
    233 || '''10 Myr''' || [[Image(s0_101myr0000.png, 90%)]] || [[Image(s15_101myr0000.png, 90%)]] || [[Image(s30_101myr0000.png, 90%)]] || [[Image(s60_101myr0000.png, 90%)]] ||
    234 || '''20 Myr''' || [[Image(s0_202myr0000.png, 90%)]] || [[Image(s15_202myr0000.png, 90%)]] || [[Image(s30_202myr0000.png, 90%)]] || [[Image(s60_202myr0000.png, 90%)]] ||
    235 || '''27 Myr''' || [[Image(s0_273myr0000.png, 90%)]] || [[Image(s15_273myr0000.png, 90%)]] || [[Image(s30_273myr0000.png, 90%)]] || [[Image(s60_273myr0000.png, 90%)]] ||
     226|| '''0 Myr''' || [[Image(s0_0myr0000.png, width=400)]] || [[Image(s15_0myr0000.png, width=400)]] || [[Image(s30_0myr0000.png, width=400)]] || [[Image(s60_0myr0000.png, width=400)]] ||
     227|| '''10 Myr''' || [[Image(s0_101myr0000.png, width=400)]] || [[Image(s15_101myr0000.png, width=400)]] || [[Image(s30_101myr0000.png, width=400)]] || [[Image(s60_101myr0000.png, width=400)]] ||
     228|| '''20 Myr''' || [[Image(s0_202myr0000.png, width=400)]] || [[Image(s15_202myr0000.png, width=400)]] || [[Image(s30_202myr0000.png, width=400)]] || [[Image(s60_202myr0000.png, 90%)]] ||
     229|| '''27 Myr''' || [[Image(s0_273myr0000.png, width=400)]] || [[Image(s15_273myr0000.png, width=400)]] || [[Image(s30_273myr0000.png, width=400)]] || [[Image(s60_273myr0000.png, width=400)]] ||
    236230}}}
    237231[[CollapsibleEnd]]
    238232
    239233[[CollapsibleStart(Spectra Table: Run vs. Energy)]]
    240 
    241 [[Image(01232015-spectra_table_tevol.png, 75%)]]
    242 
     234[[Image(01232015-spectra_table_tevol.png, width=1000)]]
    243235{{{#!comment
    244236|| '''Run-Energy''' || '''Gravitational''' || '''Magnetic''' || '''Kinetic''' || '''v^2'' ||
    245 || '''Shear 0''' || [[Image(S0_Gravitational0000.png, 90%)]] || [[Image(S0_Magnetic0000.png, 90%)]] || [[Image(S0_Kinetic0000.png, 90%)]] || [[Image(S0_vxtotal0000.png, 90%)]] ||
    246 || '''Shear 15''' || [[Image(S15_Gravitational0000.png, 90%)]] || [[Image(S15_Magnetic0000.png, 90%)]] || [[Image(S15_Kinetic0000.png, 90%)]] || [[Image(S15_vxtotal0000.png, 90%)]] ||
    247 || '''Shear 30''' || [[Image(S30_Gravitational0000.png, 90%)]] || [[Image(S30_Magnetic0000.png, 90%)]] || [[Image(S30_Kinetic0000.png, 90%)]] || [[Image(S30_vxtotal0000.png, 90%)]] ||
    248 || '''Shear 60''' || [[Image(S60_Gravitational0000.png, 90%)]] || [[Image(S60_Magnetic0000.png, 90%)]] || [[Image(S60_Kinetic0000.png, 90%)]] || [[Image(S60_vxtotal0000.png, 90%)]] ||
     237|| '''Shear 0''' || [[Image(S0_Gravitational0000.png, width=400)]] || [[Image(S0_Magnetic0000.png, width=400)]] || [[Image(S0_Kinetic0000.png, width=400)]] || [[Image(S0_vxtotal0000.png, width=400)]] ||
     238|| '''Shear 15''' || [[Image(S15_Gravitational0000.png, width=400)]] || [[Image(S15_Magnetic0000.png, width=400)]] || [[Image(S15_Kinetic0000.png, width=400)]] || [[Image(S15_vxtotal0000.png, width=400)]] ||
     239|| '''Shear 30''' || [[Image(S30_Gravitational0000.png, width=400)]] || [[Image(S30_Magnetic0000.png, width=400)]] || [[Image(S30_Kinetic0000.png, width=400)]] || [[Image(S30_vxtotal0000.png, width=400)]] ||
     240|| '''Shear 60''' || [[Image(S60_Gravitational0000.png, width=400)]] || [[Image(S60_Magnetic0000.png, width=400]] || [[Image(S60_Kinetic0000.png, width=400)]] || [[Image(S60_vxtotal0000.png, width=400)]] ||
    249241}}}
    250 
    251 [[CollapsibleEnd]]
    252 
     242[[CollapsibleEnd]]
    253243[[CollapsibleEnd]]
    254244
    255245[[CollapsibleStart(Column Density & Inverse Beta Maps)]]
    256 
    257246||  || '''[https://astrobear.pas.rochester.edu/trac/wiki/u/erica/CF_coldens Column Density Map] with Sinks''' (left) '''[https://astrobear.pas.rochester.edu/trac/wiki/u/erica/CF_BetaMaps Inverse Beta Maps]''' (right) ||
    258 || '''Shear 0''' || [[Image(s0cdm-02062015.png)]] || [[Image(s0invbeta-02062015.png)]] ||
    259 || '''Shear 15''' || [[Image(s15cdm-02062015.png)]] || [[Image(s15invbeta-02062015.png)]] ||
    260 || '''Shear 30''' || [[Image(s30cdm-02062015.png)]] || [[Image(s30invbeta-02062015.png)]] ||
    261 || '''Shear 60''' || [[Image(s60cdm-02062015.png)]] || [[Image(s60invbeta-02062015.png)]] ||
    262 [[CollapsibleEnd]
     247|| '''Shear 0''' || [[Image(s0cdm-02062015.png, width=400)]] || [[Image(s0invbeta-02062015.png, width=400)]] ||
     248|| '''Shear 15''' || [[Image(s15cdm-02062015.png, width=400)]] || [[Image(s15invbeta-02062015.png, width=400)]] ||
     249|| '''Shear 30''' || [[Image(s30cdm-02062015.png, width=400)]] || [[Image(s30invbeta-02062015.png, width=400)]] ||
     250|| '''Shear 60''' || [[Image(s60cdm-02062015.png, width=400)]] || [[Image(s60invbeta-02062015.png, width=400)]] ||
     251[[CollapsibleEnd]]
    263252
    264253[[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.
    265254
    266 || '''Shear 0''' || [[Image(S0_BvnFigure.png, 70%)]] ||
    267 || '''Shear 15''' || [[Image(S15_BvnFigure.png, 70%)]] ||
    268 || '''Shear 30''' || [[Image(S30_BvnFigure.png, 70%)]] ||
    269 || '''Shear 60''' || [[Image(S60_BvnFigure.png, 90%)]] ||
    270 
     255|| '''Shear 0''' || [[Image(S0_BvnFigure.png, width=800)]] ||
     256|| '''Shear 15''' || [[Image(S15_BvnFigure.png, width=800)]] ||
     257|| '''Shear 30''' || [[Image(S30_BvnFigure.png, width=800)]] ||
     258|| '''Shear 60''' || [[Image(S60_BvnFigure.png, width=1000)]] ||
    271259[[CollapsibleEnd]]
    272260