Changes between Version 3 and Version 4 of AstroBearProjects/MagnetizedClumpsNS


Ignore:
Timestamp:
01/07/14 20:40:19 (11 years ago)
Author:
Shule Li
Comment:

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  • AstroBearProjects/MagnetizedClumpsNS

    v3 v4  
    118118Since the force free field can be add up and maintain the force free property, we can achieve broad spectrum by adding in a large number of spherical force free fields with various frequencies.[[BR]]
    119119Given an initial field, we can also decompose it into the combination of eigenfunctions and then find out a cancelling field to obtain a force free state.[[BR]]
    120 
    121 = Magnetized Cloud Runs =
    122 
    123 The Magnetic Clump Simulations:[[BR]][[BR]]
    124 Click the following links for animations.[[BR]]
    125 [http://www.pas.rochester.edu/~shuleli/currentsheet/den_b01_nr.gif GIF:Density, Beta 0.1, non resistive][[BR]]
    126 [http://www.pas.rochester.edu/~shuleli/currentsheet/den_b10_nr.gif GIF:Density, Beta 1.0, non resistive][[BR]]
    127 [http://www.pas.rochester.edu/~shuleli/currentsheet/den_b10_r.gif GIF:Density, Beta 1.0, resistive][[BR]][[BR]]
    128 [http://www.pas.rochester.edu/~shuleli/currentsheet/mag_b01_nr.gif GIF:Magnetic Pressure, Beta 0.1, non resistive][[BR]]
    129 [http://www.pas.rochester.edu/~shuleli/currentsheet/mag_b10_r.gif GIF:Magnetic Pressure, Beta 1.0, resistive][[BR]]
    130 [http://www.pas.rochester.edu/~shuleli/currentsheet/mc01nr.gif GIF:Density, Beta 0.1, non resistive (Periodic BC)][[BR]]
    131 [http://www.pas.rochester.edu/~shuleli/currentsheet/mc01nrb.gif GIF:Magnetic Pressure, Beta 0.1, non resistive (Periodic BC)][[BR]]
    132 [http://www.pas.rochester.edu/~shuleli/currentsheet/rc01r.gif GIF:Density, Beta 0.1, resistive (Periodic BC)][[BR]]
    133 [http://www.pas.rochester.edu/~shuleli/currentsheet/rc01rb.gif GIF:Magnetic Pressure, Beta 0.1, resistive (Periodic BC)][[BR]]
    134 [[Image(http://www.pas.rochester.edu/~shuleli/MagCloud/Mag_Clump.png, 40%)]][[BR]][[BR]]
    135 
    136 [[BR]][[BR]]
    137 [[Image(http://www.pas.rochester.edu/~shuleli/MC50/MC1116.png, 50%)]][[BR]][[BR]]
    138 
    139 [[Image(http://www.pas.rochester.edu/~shuleli/MC50/MCH001.png, 50%)]][[BR]][[BR]]
    140 
    141 
    142 [http://www.pas.rochester.edu/~shuleli/MC50/MC001.gif GIF: 0.1 NR][[BR]]
    143 [http://www.pas.rochester.edu/~shuleli/MC50/MC010.gif GIF: 1 NR][[BR]]
    144 [http://www.pas.rochester.edu/~shuleli/MC50/MC100.gif GIF: 10 NR][[BR]]
    145 
    146 
    147 [http://www.pas.rochester.edu/~shuleli/MC50/RC001.gif GIF: 0.1 R][[BR]]
    148 [http://www.pas.rochester.edu/~shuleli/MC50/RC010.gif GIF: 1 R][[BR]]
    149 [http://www.pas.rochester.edu/~shuleli/MC50/RC100.gif GIF: 10 R][[BR]]
    150 
    151 
    152 [http://www.pas.rochester.edu/~shuleli/MC50/MCH001.gif GIF: 0.1 NR 2AMR][[BR]]
    153 
    154 
    155 [[BR]][[BR]]
    156 Updated 11/21/2011[[BR]][[BR]]
    157 The Morphological Evolution of beta = 0.1 Magnetized Clump:[[BR]]
    158 The second row shows the magnetic beta (inverted), the purple region is where beta < 1. [[BR]][[BR]]
    159 [[Image(http://www.pas.rochester.edu/~shuleli/1121/ClumpMorph.png, 50%)]][[BR]][[BR]]
    160 
    161 
    162 [[BR]][[BR]]
    163 Updated 12/21/2011[[BR]][[BR]]
    164 Field Spectrum Impact [[BR]][[BR]]
    165 [[Image(http://www.pas.rochester.edu/~shuleli/ClumpStudy/cloudstudy1.png, 40%)]][[BR]][[BR]]
    166 [[Image(http://www.pas.rochester.edu/~shuleli/ClumpStudy/cloudstudy2.png, 40%)]][[BR]][[BR]]
    167