Microphysical Diversity in Two Very Closely Spaced Magnetic Switchbacks Observed by Parker Solar Probe
physics.space-ph, astro-ph.SR
Submitted: 2026-09-17
Updated: 2026-09-17
Comments: 26 pages, 9 figures, 1 table. Accepted for publication in Physical Review D
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Switchbacks in the near-Sun magnetic field: long memory and impact on the turbulence cascade
- Parker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum
- Switchbacks as signatures of magnetic flux ropes generated by interchange reconnection in the corona
- On the formation of solar wind & switchbacks, and quiet Sun heating
- In-situ switchback formation in the expanding solar wind
- Magnetic field kinks and folds in the solar wind
- Shear-Driven Transition to Isotropically Turbulent Solar Wind Outside the Alfven Critical Zone
- The Structure and Origin of Switchbacks: Parker Solar Probe Observations
- Intermittent Dissipation and Local Heating in the Solar Wind
- Magnetic Switchback Occurrence Rates in the Inner Heliosphere: Parker Solar Probe and 1 au
- Association of intermittency with electron heating in the near-Sun solar wind
- Multiscale Solar Wind Turbulence Properties inside and near Switchbacks measured by Parker Solar Probe
- Anisotropic scaling of magnetohydrodynamic turbulence
- Statistical analysis of intermittency and its association with proton heating in the near Sun environment
- Scattering of Strahl Electrons in the Solar Wind between 0.3 and 1 au: Helios Observations
- Electron Strahl and Halo Formation in the Solar Wind
- Applicability of Taylor's Hypothesis during Parker Solar Probe perihelia
- A Model of Turbulence in Magnetized Plasmas: Implications for the Dissipation Range in the Solar Wind
- Imprints of expansion onto the local anisotropy of solar wind turbulence