Changes between Version 37 and Version 38 of AstroBearProjects

Timestamp:

07/18/11 14:30:22 (14 years ago)

Author:

Shule Li

Comment:

—

AstroBearProjects

@@ -64 +64 @@
 
 
-'''wiki:AstroBearProjects/AblativeRT Ablative RT] (Shule, Kris. [RochesterGroup University of Rochester])'''
+'''[wiki:AstroBearProjects/AblativeRT Ablative RT] (Shule, Kris. [RochesterGroup University of Rochester])'''
  * Modelling multi-mode perturbation 3D Rayleigh-Taylor instability with ablation effects. The [LinSolve Linear System Solver] was previously used to handle heat conduction/diffusion effects, and the nonlinear dependence on temperature is suitable for laboratory experiments. When HYPRE is fully integrated into AstroBEAR, it will handle the diffusion process.
 
@@ -83 +83 @@
  * 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. 
  * 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.
+
+'''[wiki:AstroBearProjects/stardisruption Star Disruption] (Xiaoyue, Jason, Shule, [RochesterGroup University of Rochester], University of Virginia)'''
+ * Studying the tidal disruption of stellar objects around intermediate and massive black holes.
+
+'''[wiki:AstroBearProjects/resistiveMHD Resistive MHD] (Shule, [RochesterGroup University of Rochester])'''
+ * Testing the resistive MHD functionality.
+
+