Changes between Version 53 and Version 54 of CollidingFlows


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Timestamp:
10/17/12 10:16:00 (12 years ago)
Author:
Jonathan
Comment:

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  • CollidingFlows

    v53 v54  
    114114[[Image(PowerSpectraSmooth0.png, width=400)]]
    115115
    116 It is good to see that the spectra agree quite well at resolved wave lengths and that with each additional level of data, you extend the spectra to higher wave numbers.  Also the rise at the end of the spectra (as well as the smaller one to the left) coincide with the maximum resolvable wavelength which coincides with the cell size of the next coarser grid.  Regions that have gradients but are not resolved to the finest level will have a stair-step signal, where each step has 2 points (or 4, or 8 points).  This will lead to power with wavelengths corresponding to the nyquist frequency, or twice, four times, etc...  On the first frame - the only place where there are gradients that are not completely refined - are at the edges of the colliding flow - where there is a good amount of shear.  This is verified below where the initial spike at the nyquist frequency is dominated by solenoidal terms and not compressive terms.
     116It is good to see that the spectra agree quite well at resolved wave lengths and that with each additional level of data, you extend the spectra to higher wave numbers.  Also the rise at the end of the spectra (as well as the smaller one to the left) coincide with the maximum resolvable wavelength which coincides with the cell size of the next coarser grid.  Regions that have gradients but are not resolved to the finest level will have a stair-step signal, where each step has 2 points (or 4, or 8 points).  This will lead to power with wavelengths corresponding to the nyquist frequency, or twice, four times, etc...  On the first frame - the only place where there are gradients that are not completely refined - are at the edges of the colliding flow (circled below) - where there is a good amount of shear.  This is verified below where the initial spike at the nyquist frequency is dominated by solenoidal terms and not compressive terms.
    117117
    118118[[Image(InitialVelocityField.png, width=400)]]
     
    122122----
    123123
    124 Below were taken from a region 80x80x20 with a radial cosine window (ellipsoid)
    125 so it includes shear with ambient...  Also the fact that the box is not cubic - leads to different wavenumbers (normalized to the longest mode 80 pc).  While the ky and kz wavenumbers go like 1, 2, 3, 4... the kx wave numbers go like 4, 8, 12, 16, and so on...  This means that if we sample radial bins with a width of 1, we will have over sampling the kx modes - which leads to the sawtooth pattern that was not seen above.
     124The following were taken from a region 80x80x20 with a radial cosine window (ellipsoid)
     125so it includes shear with ambient...  Also the fact that the box is not cubic - leads to different wavenumbers (normalized to the longest mode 80 pc).  While the ky and kz wavenumbers go like 1, 2, 3, 4... the kx wave numbers go like 4, 8, 12, 16, and so on...  This means that if we sample radial bins with a width of 1, we will have over sampling the kx modes - which leads to the sawtooth pattern that was not seen above. This can be corrected if we switch to a 40x40x40 window.
    126126
    127127
     
    140140
    141141Kinetic Energy Spectra [attachment:Kinetic.gif gif] and [attachment:Kinetic.AVI avi]
     142(Left is smooth and Right is clumpy.  Lines are solenoidal kinetic energy, compressive kinetic energy, the x-contribution to the kinetic energy, and the total kinetic energy spectra.)
     143
    142144|| 0 Myr ||  [[Image(Kinetic0000.bmp, width=400)]]  ||
    143145|| 10 Myr || [[Image(Kinetic0083.bmp, width=400)]]  ||
     
    145147|| 27 Myr || [[Image(Kinetic0245.bmp, width=400)]]  ||
    146148
     149
     150Velocity Spectra [attachment:Spectra.gif gif] and [attachment:Spectra.AVI avi]
     151(Same as for Kinetic Energy Spectra)
     152|| 0 Myr ||  [[Image(Spectra0000.bmp, width=400)]]  ||
     153|| 10 Myr || [[Image(Spectra0083.bmp, width=400)]]  ||
     154|| 20 Myr || [[Image(Spectra0166.bmp, width=400)]]  ||
     155|| 27 Myr || [[Image(Spectra0245.bmp, width=400)]]  ||
     156
     157
    147158Mass and Grav Energy Spectra [attachment:MassGrav.gif gif] and [attachment:MassGrav.AVI avi]
     159
     160(Left is Mass and Right is GravEnergy.  Blue line is clumpy and red line is smooth.)
     161
    148162|| 0 Myr ||  [[Image(MassGrav0000.bmp, width=400)]]  ||
    149163|| 10 Myr || [[Image(MassGrav0083.bmp, width=400)]]  ||
    150164|| 20 Myr || [[Image(MassGrav0166.bmp, width=400)]]  ||
    151165|| 27 Myr || [[Image(MassGrav0245.bmp, width=400)]]  ||
    152 
    153 Velocity Spectra [attachment:Spectra.gif gif] and [attachment:Spectra.AVI avi]
    154 || 0 Myr ||  [[Image(Spectra0000.bmp, width=400)]]  ||
    155 || 10 Myr || [[Image(Spectra0083.bmp, width=400)]]  ||
    156 || 20 Myr || [[Image(Spectra0166.bmp, width=400)]]  ||
    157 || 27 Myr || [[Image(Spectra0245.bmp, width=400)]]  ||
    158166
    159167[[CollapsibleStart(Previous runs)]]