Monday, 25 February 2019
Dr Robert L. Lysak
University of Minnesota
"Alfvén Waves and the Aurora"
The aurora borealis and aurora australis are produced by the impact of energetic electrons and protons on the high-altitude atmosphere. How these particles become energized and accelerated toward the Earth is a subject of ongoing research. The ultimate energy source for the aurora on Earth is the interaction of the solar wind with the Earth’s magnetosphere, the region in which the geomagnetic field controls the dynamics. However, satellite observations show that the auroral acceleration process occurs rather close to Earth, at altitudes of about 6000 km. The energy from the solar wind-magnetosphere interaction is carried to the acceleration by Alfvén waves, after their discoverer, the Swedish scientist Hannes Alfvén. The Alfvén waves are guided along the magnetic field, making a natural transmission line that carries energy toward the Earth. Auroral particle acceleration takes on at least two different forms: a quasi-static acceleration that produces electrons of nearly constant energy, and a dynamic acceleration process that produces a broad spectrum of waves. This latter form is now known to be associated with direct acceleration of the particles by the Alfvén waves. The aurora is also seen on other planets, most notable at Jupiter, where the auroral acceleration processes are now being observed by NASA’s Juno satellite in polar orbit around Jupiter. The Juno observations show some similar features to those at Earth but also some intriguing differences. Study of the aurora in these different environments is leading to a better understanding of these beautiful and mysterious lights in the polar night sky.
WHEN: Monday 25 February 2019
WHERE: Room 314, Science 3 Building
TIME: 3.00 pm–4.00 pm
All interested are welcome to attend
Light refreshments to follow in Common Room