blue, red, and green computer-generated graphic.

Computer simulation of a burning front moving upward through a channel distorted by strong turbulence. This burning front is similar to that which incinerates a star in about a second during a thermonuclear supernova. The red surface is the forward side of the front and the blue is the back. Simulation by UA faculty member Dean Townsley.

IceCube neutrino observatory
High Energy Physics Seminar

December 4 @ 2:00 pm

External speakers: Landsteiner (Oct 2, 2020), Takayanagi (Dec 4, 2020)

See Event Details

IceCube neutrino observatory
High Energy Physics Seminar

December 11 @ 2:00 pm

External speakers: Landsteiner (Oct 2, 2020), Takayanagi (Dec 4, 2020)

See Event Details