IPELS: Plasma dynamics

Chair: Paul Bellan, California Institute of Technology

14:00 - 14:20  The dynamics of supersonic plasma flows interaction with the magnetic arch in a laboratory setup.

14:20 - 14:40  Importance of axi-symmetry of the 1/1 kink mode (2-D or 3-D) in determination of the reconnection time scales in the sawtooth instability.

14:40 - 14:55  An MHD Modeling of the initiation and Dynamics of the X9.3 Flare Observed in September 2017.

14:55 - 15:10  Intermittent evolution of heliospheric magnetized structures: from Solar Braids to Magnetic Knots.

15:10 - 15:25  Non-local generation of plasma in a magnetic nozzle.

15:25 - 15:40  Three-dimensional MHD turbulence reconnection by coupling among multiple tearing layers.

The dynamics of supersonic plasma flows interaction with the magnetic arch in a laboratory setup

Mikhail Viktorov, Institute of Applied Physics of Russian Academy of Sciences, Russia

Importance of axi-symmetry of the 1/1 kink mode (2-D or 3-D) in determination of the reconnection time scales in the sawtooth instability

Hyeon K. Park, UNIST, South Korea

An MHD Modeling of the initiation and Dynamics of the X9.3 Flare Observed in September 2017

Satoshi Inoue, Institute for Space-Earth Environmental Research, Nagoya University, Japan

Yumi Bamba , Institute for Advanced Research, Nagoya University/Instiute for Space-Earth Environmental Research, Nagoya Univresity, Japan

Intermittent evolution of heliospheric magnetized structures: from Solar Braids to Magnetic Knots

Ilan Roth, University of California, Berkeley, CA, United States

Non-local generation of plasma in a magnetic nozzle.

Alex Bennet, Australian National University, Australia

Rod Boswell, Australian National University, Australia

Christine Charles, Australian National University, Australia

Three-dimensional MHD turbulence reconnection by coupling among multiple tearing layers

Shuoyang Wang, The University of Tokyo, Japan

Takaaki Yokoyama, The University of Tokyo, Japan