activity
20172021
most citedPhysics-constrained, low-dimensional models for MHD: First-principles and data-driven approaches

99 citations · 176 across the 6 of their papers we have counts for

collaborators

6 papers

physics.plasm-ph2021★ 4 cited

The structure of global conservation laws in Galerkin plasma models

Alan A. Kaptanoglu, Kyle D. Morgan, Christopher J. Hansen +1

Plasmas are highly nonlinear and multi-scale, motivating a hierarchy of models to understand and describe their behavior. However, there is a scarcity of plasma models of lower fid…

physics.comp-ph2020★ 99 cited

Physics-constrained, low-dimensional models for MHD: First-principles and data-driven approaches

Alan A. Kaptanoglu, Kyle D. Morgan, Chris J. Hansen +1

Plasmas are highly nonlinear and multi-scale, motivating a hierarchy of models to understand and describe their behavior. However, there is a scarcity of plasma models of lower fid…

physics.plasm-ph2020★ 4 cited

Advanced modeling for the HIT-SI Experiment

Alan A. Kaptanoglu, Thomas E. Benedett, Kyle D. Morgan +2

A two-temperature magnetohydrodynamic (MHD) model, which evolves the electron and ion temperatures separately, is implemented in the PSI-Tet code and used to model plasma dynamics…

physics.plasm-ph2019★ 67 cited

Characterizing Magnetized Plasmas with Dynamic Mode Decomposition

Alan A. Kaptanoglu, Kyle D. Morgan, Chris J. Hansen +1

Accurate and efficient plasma models are essential to understand and control experimental devices. Existing magnetohydrodynamic or kinetic models are nonlinear, computationally int…

astro-ph.SR2018

Self-organization of solar magnetic fields

T. R. Jarboe, T. E. Benedett, C. J. Everson +6

Self-organization properties of sustained magnetized plasma are applied to selected solar data to understand solar magnetic fields. Torsional oscillations are speed-up and slow-dow…

astro-ph.SR2017★ 2 cited

Evidence for a shallow thin magnetic structure and solar dynamo: the driver of torsional oscillations

T. R. Jarboe, T. E. Benedett, C. J. Everson +6

The solar dynamo and the solar Global internal Magnetic Structure (GMS) appear to be a thin (2 Mm thick) structure near (1 Mm below) the solar surface. Evidence for the…