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Session 104 - IGM.
Display session, Thursday, January 16
We have combined a particle based fluid dynamics code (SPH) with grid based magnetohydrodynamics and gravity solvers to develop a flexible numerical tool for exploring a wide variety of astrophysical problems in which MHD is important. With simulations of the intergalactic medium at z \simeq 3 we explore the role that gas flows play in amplifying seed magnetic fields of various sorts.
Program listing for Thursday