Changes between Version 38 and Version 39 of AstroBearProjects/resistiveMHD
- Timestamp:
- 01/07/14 20:38:11 (11 years ago)
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AstroBearProjects/resistiveMHD
v38 v39 205 205 Constant 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]] 206 206 207 [[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]] 208 208 209 209 Here is a movie for it:[[BR]] … … 212 212 The following figure is the "By" (magnetic field perpendicular to the shock normal) case at around 3 clump crushing time scales.[[BR]][[BR]] 213 213 214 [[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]] 215 215 216 216 Here is a movie for it:[[BR]] … … 220 220 221 221 Spitzer resistivity, Comparison animation for beta = 1, 10 and infinite: [[BR]] 222 [[Image(hydronew.png, 50%)]][[BR]][[BR]]222 [[Image(hydronew.png, 40%)]][[BR]][[BR]] 223 223 224 224 http://www.pas.rochester.edu/~shuleli/NLUF_sep/movieall.gif [[BR]][[BR]]