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physics.space-ph2026
Transport of electrons in tangled magnetic fields
Daniel Verscharen, Natasha Jeffrey, Anton Artemyev +6
Cosmic magnetic fields are typically inhomogeneous and often highly tangled due to large-scale plasma flows, turbulence, and instabilities. If the variations in the magnetic field…
physics.space-ph2025
Langmuir Wave Excitation in Solar-wind Magnetic Holes
Jingting Liu, Daniel Verscharen, Jesse Coburn +8
Magnetic holes are structures commonly observed in various space plasma environments throughout the solar system, including the solar wind. These structures are characterized by a…