Changes between Version 41 and Version 42 of AstroBearProjects/MagnetizedClumps


Ignore:
Timestamp:
01/07/14 21:34:20 (11 years ago)
Author:
Shule Li
Comment:

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  • AstroBearProjects/MagnetizedClumps

    v41 v42  
    9393
    9494The mathematical model that can qualitatively explain the line plots is available in the paper:[[BR]]
     95Magnetohydrodynamic Shock-Clump Evolution with Self-contained Magnetic Fields, Shule Li, Adam Frank, Eric Blackman, Astrophys Journal 774 (2013), 133-149
     96[[BR]][[BR]]
    9597
    96 [[BR]][[BR]]
     98== Random Field Configuration ==
     99We have started investigating the contained field interaction with shock when the field is random (with a certain known spectrum). [[BR]][[BR]]
     100[[Image(http://www.pas.rochester.edu/~shuleli/HedlaPics/fieldscale2.png, 50%)]]
     101
    97102== Presentations ==
    98103