Todd Elder
Research Subjects
Todd Elder has a total of 16 co-authors. Here are the top co-authors by number of shared publications:
- Allen H. Boozer
Columbia University
3 shared publications - Antoinne Baillod
Department of Applied Physics and Applied Mathematics, Columbia University, New York, NY 10027, United States of America
1 shared publication - Charles P. S. Swanson
Thea Energy, Inc., Kearny, NJ, USA
1 shared publication - Christopher Berg Smiet
École Polytechnique Fédérale de Lausanne
1 shared publication - Daniel William Dudt
Princeton University, Princeton, NJ 08544, USA
1 shared publication - David A. Gates
Princeton Plasma Phys Lab, Princeton, NJ 08543 USA
1 shared publication
Latest Publications
- Open Access
- 1 July 2026
- Published by Elsevier in Fusion Engineering and Design
- Vol. 230
Planar coil design for the Helios stellarator fusion power plant
- 1 July 2026
- Published by Elsevier in Fusion Engineering and Design
- Vol. 230
Open AccessPlanar coil design for the Helios stellarator fusion power plant
- Open Access
- 4 May 2026
- Published by Cambridge University Press (CUP) in Journal of Plasma Physics
- Vol. 92 (2)
Stellarator divertor design by optimising coils for surfaces with sharp corners
In stellarators, achieving effective divertor configurations is challenging due to the three-dimensional nature of the magnetic fields, which often leads to chaotic field lines and separatrices surrounded by a thick stochastic layer. This work presents a novel approach to directly optimise modular stellarator coils for a sharp X-point divertor topology akin to the Large Helical Device’s (LHD) helical divertor using a target plasma surface with sharp corners. By minimising the normal magnetic field component on this surface, we construct a clean separatrix with minimal chaos. Notably, this approach demonstrates the first LHD-like helical divertor design using optimised modular coils instead of helical coils. Separatrices are produced with significantly lower chaos than in LHD, demonstrating that a wide chaotic layer is not intrinsic to the helical divertor. Additional optimisation methods are implemented to improve engineering feasibility of the coils and reduce chaos, including weighted quadrature and manifold optimisation, a method which does not rely on normal field minimisation. The results outline several new strategies for divertor design in stellarators, although it remains to achieve these edge divertor features at the same time as internal field qualities like quasisymmetry.
- 4 May 2026
- Published by Cambridge University Press (CUP) in Journal of Plasma Physics
- Vol. 92 (2)
Open AccessStellarator divertor design by optimising coils for surfaces with sharp corners
In stellarators, achieving effective divertor configurations is challenging due to the three-dimensional nature of the magnetic fields, which often leads to chaotic field lines and separatrices surrounded by a thick stochastic layer. This work presents a novel approach to directly optimise modular stellarator coils for a sharp X-point divertor topology akin to the Large Helical Device’s (LHD) helical divertor using a target plasma surface with sharp corners. By minimising the normal magnetic field component on this surface, we construct a clean separatrix with minimal chaos. Notably, this approach demonstrates the first LHD-like helical divertor design using optimised modular coils instead of helical coils. Separatrices are produced with significantly lower chaos than in LHD, demonstrating that a wide chaotic layer is not intrinsic to the helical divertor. Additional optimisation methods are implemented to improve engineering feasibility of the coils and reduce chaos, including weighted quadrature and manifold optimisation, a method which does not rely on normal field minimisation. The results outline several new strategies for divertor design in stellarators, although it remains to achieve these edge divertor features at the same time as internal field qualities like quasisymmetry.
- Open Access
- 25 July 2025
- Published by IOP Publishing in Nuclear Fusion
- Vol. 65 (8) , 086040
Enhancing stellarator accessibility through port size optimization
Access to the plasma chamber in a stellarator reactor is essential for maintenance and diagnostics. However, the complex geometry of stellarator coils, often characterized by their strong twisting, can severely limit the space available for access ports. This study introduces a novel optimization approach in which access ports are represented as closed curves on the plasma boundary. By carefully selecting a set of objectives and penalties related to the access port, we demonstrate the first stellarator coil optimization explicitly targeting improved access port size. The trade-off between magnetic field quality and port size is analyzed through the Pareto front of their respective objectives. The optimal location of a port is explained using a current potential approach. Finally, we show that additional shaping coils, such as windowpane coils, can enable the crossing of the Pareto front to achieve superior configurations.
- 25 July 2025
- Published by IOP Publishing in Nuclear Fusion
- Vol. 65 (8) , 086040
Open AccessEnhancing stellarator accessibility through port size optimization
Access to the plasma chamber in a stellarator reactor is essential for maintenance and diagnostics. However, the complex geometry of stellarator coils, often characterized by their strong twisting, can severely limit the space available for access ports. This study introduces a novel optimization approach in which access ports are represented as closed curves on the plasma boundary. By carefully selecting a set of objectives and penalties related to the access port, we demonstrate the first stellarator coil optimization explicitly targeting improved access port size. The trade-off between magnetic field quality and port size is analyzed through the Pareto front of their respective objectives. The optimal location of a port is explained using a current potential approach. Finally, we show that additional shaping coils, such as windowpane coils, can enable the crossing of the Pareto front to achieve superior configurations.
- Open Access
- 1 October 2024
- Published by AIP Publishing in Physics of Plasmas
- Vol. 31 (10)
Current potential patches
A novel form of the current potential, a mathematical tool for the design of stellarators and stellarator coils, is developed. Specifically, these are current potentials with a finite-element basis, called current potential patches. Current potential patches leverage the relationship between distributions of magnetic dipoles and current potentials to explore limits of the access properties of stellarator coil sets. An example calculation is shown using the Helically Symmetric Experiment (HSX) equilibrium, demonstrating the method's use in coil design and understanding the limits of the access properties of coil sets. Current potential patches have additional desirable properties such as of promoting sparse current sheet solutions and identifying crucial locations of shaping current placement. A result is found for the HSX equilibrium that shaping currents covering only 22% of the winding surface are sufficient to produce the equilibrium to a good accuracy, provided a toroidal field is generated by an exterior coil set.
- 1 October 2024
- Published by AIP Publishing in Physics of Plasmas
- Vol. 31 (10)
Open AccessCurrent potential patches
A novel form of the current potential, a mathematical tool for the design of stellarators and stellarator coils, is developed. Specifically, these are current potentials with a finite-element basis, called current potential patches. Current potential patches leverage the relationship between distributions of magnetic dipoles and current potentials to explore limits of the access properties of stellarator coil sets. An example calculation is shown using the Helically Symmetric Experiment (HSX) equilibrium, demonstrating the method's use in coil design and understanding the limits of the access properties of coil sets. Current potential patches have additional desirable properties such as of promoting sparse current sheet solutions and identifying crucial locations of shaping current placement. A result is found for the HSX equilibrium that shaping currents covering only 22% of the winding surface are sufficient to produce the equilibrium to a good accuracy, provided a toroidal field is generated by an exterior coil set.
- 1 June 2021
- Published by AIP Publishing in Physics of Plasmas
- Vol. 28 (6) , 062303
Example of exponentially enhanced magnetic reconnection driven by a spatially bounded and laminar ideal flow
In laboratory and natural plasmas of practical interest, the spatial scale Δd at which magnetic field lines lose distinguishability differs enormously from the scale a of magnetic reconnection across the field lines. In the solar corona, plasma resistivity gives , which is the magnetic Reynolds number Rm. The traditional resolution of the paradox of disparate scales is for the current density j associated with the reconnecting field Brec to be concentrated by a factor of Rm by the ideal evolution, so . A second resolution is for the ideal evolution to increase the ratio of the maximum to minimum separation between pairs of arbitrary chosen magnetic field lines, , when calculated at various points in time. Reconnection becomes inevitable where . A simple model of the solar corona will be used for a numerical illustration that the natural rate of increase in time is linear for the current density but exponential for . Reconnection occurs on a timescale and with a current density enhanced by only from the ideal evolution time and from the current density . In both resolutions, once a sufficiently wide region, Δr, has undergone reconnection, the magnetic field loses static force balance and evolves on an Alfvénic timescale. The Alfvénic evolution is intrinsically ideal but expands the region in which is large.- 1 June 2021
- Published by AIP Publishing in Physics of Plasmas
- Vol. 28 (6) , 062303
Example of exponentially enhanced magnetic reconnection driven by a spatially bounded and laminar ideal flow
In laboratory and natural plasmas of practical interest, the spatial scale Δd at which magnetic field lines lose distinguishability differs enormously from the scale a of magnetic reconnection across the field lines. In the solar corona, plasma resistivity gives , which is the magnetic Reynolds number Rm. The traditional resolution of the paradox of disparate scales is for the current density j associated with the reconnecting field Brec to be concentrated by a factor of Rm by the ideal evolution, so . A second resolution is for the ideal evolution to increase the ratio of the maximum to minimum separation between pairs of arbitrary chosen magnetic field lines, , when calculated at various points in time. Reconnection becomes inevitable where . A simple model of the solar corona will be used for a numerical illustration that the natural rate of increase in time is linear for the current density but exponential for . Reconnection occurs on a timescale and with a current density enhanced by only from the ideal evolution time and from the current density . In both resolutions, once a sufficiently wide region, Δr, has undergone reconnection, the magnetic field loses static force balance and evolves on an Alfvénic timescale. The Alfvénic evolution is intrinsically ideal but expands the region in which is large.- 1 April 2021
- Published by Cambridge University Press (CUP) in Journal of Plasma Physics
- Vol. 87 (2)
Magnetic nulls in interacting dipolar fields
The prominence of nulls in reconnection theory is due to the expected singular current density and the indeterminacy of field lines at a magnetic null. Electron inertia changes the implications of both features. Magnetic field lines are distinguishable only when their distance of closest approach exceeds a distance $\varDelta _d$ . Electron inertia ensures $\varDelta _d\gtrsim c/\omega _{pe}$ . The lines that lie within a magnetic flux tube of radius $\varDelta _d$ at the place where the field strength $B$ is strongest are fundamentally indistinguishable. If the tube, somewhere along its length, encloses a point where $B=0$ vanishes, then distinguishable lines come no closer to the null than $\approx (a^2c/\omega _{pe})^{1/3}$ , where $a$ is a characteristic spatial scale of the magnetic field. The behaviour of the magnetic field lines in the presence of nulls is studied for a dipole embedded in a spatially constant magnetic field. In addition to the implications of distinguishability, a constraint on the current density at a null is obtained, and the time required for thin current sheets to arise is derived.- 1 April 2021
- Published by Cambridge University Press (CUP) in Journal of Plasma Physics
- Vol. 87 (2)
Magnetic nulls in interacting dipolar fields
The prominence of nulls in reconnection theory is due to the expected singular current density and the indeterminacy of field lines at a magnetic null. Electron inertia changes the implications of both features. Magnetic field lines are distinguishable only when their distance of closest approach exceeds a distance $\varDelta _d$ . Electron inertia ensures $\varDelta _d\gtrsim c/\omega _{pe}$ . The lines that lie within a magnetic flux tube of radius $\varDelta _d$ at the place where the field strength $B$ is strongest are fundamentally indistinguishable. If the tube, somewhere along its length, encloses a point where $B=0$ vanishes, then distinguishable lines come no closer to the null than $\approx (a^2c/\omega _{pe})^{1/3}$ , where $a$ is a characteristic spatial scale of the magnetic field. The behaviour of the magnetic field lines in the presence of nulls is studied for a dipole embedded in a spatially constant magnetic field. In addition to the implications of distinguishability, a constraint on the current density at a null is obtained, and the time required for thin current sheets to arise is derived.