Speaker
Description
During tokamak disruptions, the magnetic surfaces are broken creating large regions of chaotic magnetic field lines. The physics associated with post-disruption chaotic magnetic fields needs be understood to address force, heat, and runaway electron loading on the walls. Direct simulations are too challenging to allow parameter scans and have uncertainties that can only be addressed by a reliable physics understanding. Even an ideal instability that grows on a timescale $\tau_I$ and does not saturate at a small amplitude will lead to a breakup of the magnetic surfaces on a timescale $\sim 10\tau_I$. The ratio of the closest to the average separation between two neighboring magnetic surfaces drops until resistive diffusion across the locations of their closest approach competes with $\tau_I$. As surfaces break, regions of chaos are created. With chaos, each magnetic field line will have neighboring lines that exponentially separate from it with the distance along the line. When followed long enough, a single line will come arbitrarily close to every point in a single chaotic region. The annuli of magnetic surfaces between chaotic regions break by forming Cantori, which are toroidal surfaces punctured by pairs of inward and outward tubes of magnetic flux called turnstiles. In each chaotic region, the parallel current density divided by $B$ relaxes toward a spatial constant by shear Alfv\'en waves. The electric potential $\Phi_q$ required for quasi-neutrality produces both a diffusion coefficient that is Bohm-like, $D_q\approx T_e/eB$, and a large scale flow $\approx T_e/eB a_T$ across the magnetic field lines, where $a_T$ is the scale of the large scale difference in the electron temperature $T_e$. This diffusion and flow are important for sweeping impurities into the core of a disrupting tokamak plasma. These results follow from from general magnetic-evolution properties and from the separation of the electric field in the plasma into the sum of a divergence-free, $\vec{E}_B$, and a curl-free, $\vec{E}_q$, part. The divergence-free part of $\vec{E}$ determines the evolution of the magnetic field. The curl-free part enforces quasi-neutrality. This separation is given by a Helmholtz decomposition, which is unique if a boundary condition is given on the enclosing chamber wall. A deeper understanding of disruption experiments and simulations will clarify the roles of chaos, Alfv\'en waves, quasi-neutrality potentials, and helicity conservation not only in tokamak disruptions but also in magnetic reconnection in general---whether in the laboratory or in space. For more details, see $<$ https://arxiv.org/pdf/2404.09744 $>$. U.S. Department of Energy grants DE-FG02-03ER54696, DE-SC0018424, and DE-FG02-95ER54333 provided support.
| Speaker's title | Mr |
|---|---|
| Speaker's email address | ahb17@columbia.edu |
| Speaker's Affiliation | Columbia University, New York City |
| Member State or IGO | United States of America |
