Michael Brown, Swarthmore College
Fri., Sep. 19, 2014, 12:30 PM
Turbulent fluctuations in conventional fluids like air or water seem to have a universal statistical character. Measurements of statistical turbulence metrics in a wind tunnel or in a tidal basin seem to be the same. It is not known whether plasma turbulence is universal. The Sun launches a turbulent stream of high velocity plasma with imbedded magnetic fields into interplanetary space at about 400 km/s. Properties of this solar wind have been studied for decades and much is known about fluctuations in the velocity, density, and magnetic field. In this talk, I'll discuss measurements in a high velocity plasma wind tunnel at Swarthmore. The SSX MHD wind tunnel features flow speeds up to 100 km/s, magnetic field of 0.5 T, and temperatures of nearly a million Kelvin. Comparisons to measurements from the solar wind will be made.
See Prof. Brown's website for more information about his research.
Ben Vigoda, Gamelan Labs
Fri., Oct. 24, 2014, 12:30 PM
Abstract: coming soon.
See the Gamelan Labs website for more information.