Conference on Magnetospheres of the Outer Planets

Conference on Magnetospheres of the Outer Planets

MOP2024, University of Minnesota

The MOP conference aims to bring together experts from around the globe to present and discuss recent research on the magnetospheres of the outer planets.

DatesMonday, July 8 to Thursday, July 11 2024
Speakers
Dr. Kazuo Yoshioka
Prof. Carol Paty
Dr. Peter Kollmann
LR
Sponsors
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MOP2024
MOP2024
Prof. Ali Sulaiman

Prof. Ali Sulaiman

Assistant Professor, School of Physics and Astronomy, University of Minnesota
University of Minnesota
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Prof. Bob Lysak

Prof. Bob Lysak

Professor, School of Physics and Astronomy, University of Minnesota
University of Minnesota

My research emphasizes a fundamental theoretical understanding of the dynamics of plasmas in the Earth's magnetosphere, as well as in other planetary magnetospheres, the solar wind, and other astrophysical environments. I am particularly interested in the dynamics of the Earth's auroral regions. In these regions, strong currents flow along the magnetic field ("field-aligned currents") that are dissipated in the ionosphere and by accelerating the particles that produce the aurora. Changes in these current systems are mediated by waves called Alfven waves, which correspond to transverse fluctuations of the geomagnetic field. Although Alfven waves were first studied using magnetohydrodynamic (MHD) theory, I have approached them using a more complete kinetic theory; thus, these waves are sometimes called kinetic Alfven waves. Such waves can directly accelerate electrons into the ionosphere to produce the aurora. In addition, we are studying the ways in which these waves can evolve into quasi-static parallel electric fields that are known to be associated with discrete auroral arcs. These studies lead to an overall understanding of ultra-low-frequency (ULF) waves in the magnetosphere, especially the eigenmodes that can form due to the inhomogeneous nature of the magnetospheric plasma. Parallel electric fields are also necessary for the process called magnetic reconnection, which refers to the reorganization of the magnetic topology in thin current sheets. We study the dynamics of these processes as well. ULF waves are also important in Jupiter's magnetosphere, where they are driven by the motion of Jupiter's moon Io. Alfven waves may also be responsible for processes in the solar corona, such as solar flares, coronal mass ejections, and the heating of the corona to millions of degrees.

This work also benefits from collaboration with Senior Researcher Dr. Yan Song. Her work emphasizes the fundamental theory of particle acceleration and magnetic reconnection, emphasizing a dynamical approach that improves upon the quasi-steady descriptions often used to discuss these phenomena.

MOP2024, University of Minnesota

University of Minnesota
University of Minnesota
twin-cities.umn.edu