Changes between Version 44 and Version 45 of AstroBearProjects


Ignore:
Timestamp:
01/24/12 14:15:21 (13 years ago)
Author:
Shule Li
Comment:

Legend:

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  • AstroBearProjects

    v44 v45  
    8181 * Adding in cosmic ray diffusion and feedback to AstroBEAR.  When completed the code will be used to investigate 2-D Diffusive Shock Acceleration in Stellar Winds and Supernova Remnants.
    8282
    83 '''[wiki:AstroBearProjects/MagnetizedClumps Magnetized Clumps] (Shule, Jonathan, [RochesterGroup University of Rochester])'''
    84  * Studying the instabilities and shocked behavior of magnetized clumps and clouds in the interstellar medium. The clouds are usually filled by strong magnetic field with low beta.
     83
     84'''[wiki:AstroBearProjects/MagnetizedClumpsNS Magnetized Clumps] (Shule, Jonathan, [RochesterGroup University of Rochester])'''
     85 * Studying the instabilities of magnetized clumps and clouds in the interstellar medium. The clouds are usually filled by strong magnetic field with low beta.
    8586 * This work involves volume-filling spherical symmetric magnetic field configuration which is force free to maintain the initial equilibrium. Later, various physics processes such as self gravity and anisotropic diffusion could be added to the situation.
     87
     88
     89'''[wiki:AstroBearProjects/MagnetizedClumps Magnetized Clumps with Shocks] (Shule, Jonathan, [RochesterGroup University of Rochester])'''
     90 * Studying the shocked behavior of magnetized clumps and clouds in the interstellar medium. The clouds are usually filled by strong magnetic field with low beta.
     91 * This work involves volume-filling spherical symmetric magnetic field configuration which is force free to maintain the initial equilibrium. We also study the effect of background fields and various physics processes such as thermal conduction.
    8692
    8793'''[wiki:AstroBearProjects/stardisruption Star Disruption] (Xiaoyue, Jason, Shule, [RochesterGroup University of Rochester], University of Virginia)'''