This conference will bring together turbulence experts from a wide range of subfields in astrophysics and physics. The goal is to encourage and enhance interdisciplinary discussions and collaborations. The conference will cover many topics, including: turbulent dynamo, magnetic reconnection, plasma physics, space physics, unresolved physics and sub-grid models in numerical simulations, turbulence in the laboratory, new observational techniques for diagnosing turbulence, connecting observations and models, and astrophysical applications of magnetized turbulence (e.g. star formation, cosmic rays, accretion, galaxy formation and evolution).
The conference will consist of a three-day (April 5-7) scientific meeting and one day devoted to public outreach and observation of the eclipse (April 8). The conference will address topics such as observations of the solar eclipse, understanding of solar physics and the Sun as a probe to stellar astrophysics and related topics, such as space plasma, planetary systems, dark matter, dark energy, extra-galactic surveys, and the universe.
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