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Title: "Magnetohydrodynamic Turbulence in Astrophysical Plasmas"
Abstract: Most of the visible matter in the universe is comprised of turbulent, magnetized plasma, and turbulence plays a critical role in the evolution of many astrophysical systems, such as accretion flows and star-forming molecular clouds. Magnetohydrodynamics (MHD) provides a powerful, albeit approximate, framework for understanding astrophysical plasma turbulence, and in this talk I will present a tutorial introduction to some of the key ideas that underlie our current understanding of MHD turbulence. I will then briefly describe some recent work on MHD turbulence and its implications for an astrophysical system close to home, the solar wind.
Hosted by Professor Jens Mahlmann
Join Zoom Meeting
https://dartmouth.zoom.us/j/92751420885?pwd=QnIwN0RiSGkzMUtjQVZxRlZLMkcwQT09
Meeting ID: 927 5142 0885
Email Physics.Department@dartmouth.edu for passcode
Events are free and open to the public unless otherwise noted.