Changes between Version 38 and Version 39 of AstroBearProjects/resistiveMHD


Ignore:
Timestamp:
01/07/14 20:38:11 (11 years ago)
Author:
Shule Li
Comment:

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  • AstroBearProjects/resistiveMHD

    v38 v39  
    205205Constant resistivity (magnetic Reynolds number is fixed), "Bx" (magnetic field parallel to the shock normal) case at around 3 clump crushing time scales. The Rm labeled in the figure is the magnetic Reynolds number. The plot at the bottom is the case where the fluid is perfectly conductive (Rm is infinite). [[BR]][[BR]]
    206206
    207 [[Image(http://www.pas.rochester.edu/~shuleli/Resistive_Clump/denpara_lr__0100.png, 70%)]][[BR]][[BR]]
     207[[Image(http://www.pas.rochester.edu/~shuleli/Resistive_Clump/denpara_lr__0100.png, 40%)]][[BR]][[BR]]
    208208
    209209Here is a movie for it:[[BR]]
     
    212212The following figure is the "By" (magnetic field perpendicular to the shock normal) case at around 3 clump crushing time scales.[[BR]][[BR]]
    213213
    214 [[Image(http://www.pas.rochester.edu/~shuleli/Resistive_Clump/denperp_lr_0100.png, 70%)]][[BR]][[BR]]
     214[[Image(http://www.pas.rochester.edu/~shuleli/Resistive_Clump/denperp_lr_0100.png, 40%)]][[BR]][[BR]]
    215215
    216216Here is a movie for it:[[BR]]
     
    220220
    221221Spitzer resistivity, Comparison animation for beta = 1, 10 and infinite: [[BR]]
    222 [[Image(hydronew.png, 50%)]][[BR]][[BR]]
     222[[Image(hydronew.png, 40%)]][[BR]][[BR]]
    223223
    224224http://www.pas.rochester.edu/~shuleli/NLUF_sep/movieall.gif [[BR]][[BR]]