Changes between Version 40 and Version 41 of AstroBearProjects/MagnetizedClumps


Ignore:
Timestamp:
01/07/14 21:25:16 (11 years ago)
Author:
Shule Li
Comment:

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  • AstroBearProjects/MagnetizedClumps

    v40 v41  
    6060[[Image(fig02_rev_bw.png,40%)]][[BR]][[BR]]
    6161The contained magnetic field has a volume-average beta of 0.25. The volume rendered results for the four cases (the four columns for TA, TP, PA, PP cases, respectively). Each row corresponds to 1, 2 and 3.5 cloud crushing time.[[BR]]
    62 [[Image(fig03_rev_color.png,40%)]][[Image(fig04_rev_color.png,40%)]][[Image(fig05_rev_color.png,40%)]][[Image(fig06_rev_color.png,40%)]][[BR]][[BR]]
     62[[Image(fig03_rev_color.png,20%)]][[Image(fig04_rev_color.png,20%)]][[Image(fig05_rev_color.png,20%)]][[Image(fig06_rev_color.png,20%)]][[BR]][[BR]]
    6363Movies:[[BR]]
    6464TA case:[[BR]]
    … …  
    7575[[BR]][[BR]]
    7676The magnetic field intensity map is plotted as follows:[[BR]][[BR]]
    77 [[Image(fig11_rev_bw.png,50%)]][[BR]][[BR]]
     77[[Image(fig11_rev_bw.png,30%)]][[BR]][[BR]]
    7878
    7979The contained magnetic field geometry can influence the kinetic and magnetic energy evolution. As shown in the following plot:[[BR]][[BR]]