Saturation of magnetised plasma turbulence by propagating zonal flows

This paper demonstrates that strongly driven ion-scale turbulence in tokamak plasmas is regulated by a newly identified propagating zonal flow mode called the toroidal secondary mode, which nonlinearly shears turbulent eddies above a specific threshold to establish scaling laws for heat flux and fluctuation spectra that align with both simulations and experimental observations.

Richard Nies, Felix Parra, Michael Barnes, Noah Mandell, William DorlandWed, 11 Ma🔬 physics

Sparse identification of effective microparticle interaction potential in dusty plasma from simulation data

This paper demonstrates the application of the Sparse Identification of Nonlinear Dynamics (SINDy) method with a weak formulation to accurately identify effective microparticle interaction potentials from noisy simulation data, offering a promising approach for analyzing experimental dusty plasma systems like the PK-4 experiment.

Zachary Brooks Howe, Lorin Swint Matthews, Truell Hyde, Luca Guazzotto, Evdokiya KostadinovaWed, 11 Ma🔬 physics

Mode-Selective Laser Propagation and Absorption in Strongly Magnetized Inhomogeneous Plasma

This paper systematically investigates the propagation and collisional absorption of normally incident laser light in strongly magnetized inhomogeneous plasma, revealing that while left-hand circularly polarized waves reflect at cutoff with enhanced absorption at higher magnetic fields, right-hand polarized waves can transition into whistler modes above a critical frequency to penetrate and deposit energy deep within overdense plasma.

Kun Li, Wuhan Wu, Yuxi Li, Mingyang YuWed, 11 Ma🔬 physics

Nonlinear generation of global zonal structures in gyrokinetic simulations of TCV and ASDEX Upgrade magnetic configurations

Using gyrokinetic simulations with the ORB5 code, this study demonstrates that global zonal structures in the geodesic acoustic mode frequency range are non-linearly generated by the high-n component of turbulence in TCV and ASDEX Upgrade magnetic configurations, a mechanism confirmed by isolating the effect via antenna-driven turbulence modes.

I. Novikau, A. Biancalani, A. Bottino, E. Poli, G. D. Conway, P. Manz, L. Villard, N. Ohana, ASDEX Upgrade TeamWed, 11 Ma🔬 physics

Spherical compression of an applied magnetic field in inertial confinement fusion

This paper presents an analytic model demonstrating that ablation-driven field compression in magnetized inertial confinement fusion creates a radially bent field at the hotspot edge that negates thermal insulation benefits, while showing that an initially applied mirror field configuration yields superior performance compared to standard axial fields.

R. Spiers, A. Bose, C. A. Frank, D. J. Strozzi, J. D. Moody, C. A. Walsh, B. A. HammelWed, 11 Ma🔬 physics

An Interpretable Operator-Learning Model for Electric Field Profile Reconstruction in Discharges Based on the EFISH Method

This paper introduces Decoder-DeepONet (DDON), a novel interpretable operator-learning model that significantly outperforms previous neural network and classical methods in reconstructing electric field profiles from EFISH signals by offering superior accuracy, generalizability, and robustness to incomplete data while identifying optimal sampling windows.

Zhijian Yang, Edwin Setiadi Sugeng, Mhedine Alicherif, Tat Loon ChngWed, 11 Ma🤖 cs.LG

Imposing quasineutrality on electrostatic plasmas via the Dirac theory of constraints

This paper presents a method using Dirac's theory of constraints to systematically enforce quasineutrality and charge density conservation in electrostatic plasma models (Vlasov-Poisson and Vlasov-Ampère) by constructing generalized Dirac brackets that eliminate the electric field and introduce specific advection terms, thereby enabling a rigorous assessment of the quasineutral approximation's validity across kinetic scales.

D. A. Kaltsas, J. W. Burby, P. J. Morrison, E. Tassi, G. N. ThroumoulopoulosTue, 10 Ma🔬 physics

Effect of front surface engineering on high energy electron, X-ray and heavy ion generation from Relativistic laser interaction with thick high-Z targets

Experiments at the Scarlet Facility using a $10^{21}W/cm W/cm^2$ laser on thick tantalum targets revealed that while bare targets produced the highest MeV electron and X-ray yields, thicker front-surface coatings like foam and nanowires enhanced heavy ion acceleration, highlighting the critical role of coating density and thickness in optimizing particle generation and suggesting post-damage crater analysis as a viable method for benchmarking laser absorption.

J. Twardowski (Department of Materials Science and Engineering, The Ohio State University, Columbus, OH, USA), C. Kuz (Department of Physics, The Ohio State University, Columbus, OH, USA), A. S. Bogale (Los Alamos National Laboratory, Los Alamos, NM, USA, Center for Energy Research, University of California San Diego, La Jolla, CA, USA), Z. Su (Department of Materials Science and Engineering, The Ohio State University, Columbus, OH, USA), A. Lee (Department of Physics, The Ohio State University, Columbus, OH, USA), R. Kaur (Department of Materials Science and Engineering, The Ohio State University, Columbus, OH, USA), M. Eder (Department of Physics, The Ohio State University, Columbus, OH, USA), Y. Noor (Department of Materials Science and Engineering, The Ohio State University, Columbus, OH, USA), D. P. Broughton (Los Alamos National Laboratory, Los Alamos, NM, USA), Md Kazi Rokunuzzaman (Department of Materials Science and Engineering, The Ohio State University, Columbus, OH, USA), R. Hollinger (Electrical and Computer Engineering Dept, Colorado State University, Fort Collins, CO, USA), A. Blackston (Department of Materials Science and Engineering, The Ohio State University, Columbus, OH, USA), J. Strehlow (Los Alamos National Laboratory, Los Alamos, NM, USA), A. Baraona (Department of Physics, The Ohio State University, Columbus, OH, USA), P. Spingola (Department of Physics, The Ohio State University, Columbus, OH, USA), G. Tiscareno (Department of Physics, The Ohio State University, Columbus, OH, USA), D. Hanggi (Department of Physics, The Ohio State University, Columbus, OH, USA), B. Unzicker (Department of Physics, The Ohio State University, Columbus, OH, USA), C. -S. Wong (Los Alamos National Laboratory, Los Alamos, NM, USA), G. K. Ngirmang (National Sciences and Science Education, National Institute of Education, Nanyang Technological University, Singapore, Singapore), F. N. Beg (Center for Energy Research, University of California San Diego, La Jolla, CA, USA), D. Schumacher (Department of Physics, The Ohio State University, Columbus, OH, USA), E. Chowdhury (Department of Materials Science and Engineering, The Ohio State University, Columbus, OH, USA, Department of Electrical and Computer Engineering, The Ohio State University, Columbus, OH, USA, Department of Physics, The Ohio State University, Columbus, OH, USA)Tue, 10 Ma🔬 physics

Spatiotemporal Properties of Compressible Magnetohydrodynamic Turbulence from Space Plasma

Using multi-spacecraft observations from Earth's magnetosheath, this study provides the first quantitative evidence that compressible MHD turbulence exhibits a weak-to-strong transition specifically in slow modes, while fast modes remain weakly turbulent, thereby offering a comprehensive characterization of spatiotemporal properties across different turbulence regimes.

Siqi Zhao, Huirong Yan, Terry Z. Liu, Chuanpeng Hou, Ka Ho YuenTue, 10 Ma🔭 astro-ph

MMS Observations of Kinetic Alfvén Wave Turbulence and Steep Kinetic-Range Spectra in the Outer Plasma Sheet Boundary Layer

Using high-resolution MMS data from the outer Plasma Sheet Boundary Layer, this study characterizes Kinetic Alfvén Wave turbulence through a steep kinetic-range spectral slope and impulsive parallel electric fields, providing observational evidence for collisionless energy dissipation via direct wave-particle interactions in the magnetotail.

Mani K Chettri, Hemam D. Singh, Rupak MukherjeeTue, 10 Ma🔭 astro-ph

Compression-Driven Kinetic Instabilities in Magnetically Arrested Disks

This study employs 2D particle-in-cell simulations to demonstrate that continuous compression in magnetically arrested disk plasmas drives pressure anisotropy and triggers kinetic instabilities like the ion cyclotron and mirror modes, which regulate anisotropies and generate nonthermal energy spectra in ways that depend critically on plasma beta, temperature, and compression rates, thereby providing essential constraints for global fluid models of black hole accretion.

Vedant Dhruv, Lorenzo Sironi, Jordy Davelaar, Aaron TranTue, 10 Ma🔭 astro-ph