activity
20092026
most citedDirect evidence for magnetic reconnection at the boundaries of magnetic switchbacks with Parker Solar Probe

41 citations · 44 across the 11 of their papers we have counts for

collaborators

11 papers

physics.plasm-ph2026

Linear Growth Rate of Compressible Tearing Instability in a Force-Free Current Sheet

Chen Shi, Marco Velli

We investigate the linear growth rate of tearing instability in a resistive force-free current sheet using the linearized fully-compressible magnetohydrodynamics (MHD) equations. O…

astro-ph.SR2026

Bifurcations in the Heliosphere: Global-scale Coronal Pseudostreamer Evolution and the Creation of Secondary Heliospheric Current Sheets

Lizet S. Casillas, Benjamin J. Lynch, Victor Réville +2

The heliospheric current sheet (HCS) is the boundary between open magnetic fields of opposite polarity in the solar wind that connect back to their respective open flux regions in…

astro-ph.SR2026

Potential Solar Precursors to Magnetic Switchbacks

Durgesh Tripathi, Maria S. Madjarska, Judy Karpen +9

The origin of magnetic switchbacks-large-amplitude, spherically polarized magnetic-field fluctuations with local polarity inversions shown to be nearly ubiquitous in the inner heli…

physics.space-ph2026

Evolution and Impact of Switchbacks Throughout the Heliosphere

Alfred Mallet, Chen Shi, Anna Tenerani +23

Magnetic switchbacks are large-amplitude fluctuations in the interplanetary magnetic field, and appear frequently in the near-Sun solar wind explored recently by Parker Solar Probe…

physics.plasm-ph2026★ 1 cited

Three dimensional, spherically polarized magnetic fields

Anna Tenerani, Marco Velli

Turbulence in the solar wind is characterized by Alfvénic fluctuations that exhibit spherical polarization, a geometric condition resulting in the nearly constant magnitude of the…

astro-ph.SR2026

Magnetic switchback formation: a review of proposed mechanisms

Peter F. Wyper, Jonathan Squire, Etienne Pariat +19

Magnetic switchbacks are large amplitude deflections of the magnetic field within the solar wind. They are Alfvénic in character and so are associated with a spike in velocity and…

physics.space-ph2026

Solar Wind Classifications at Mars using Machine Learning Techniques

Catherine E. Regan, Silvia Ferro, Austin M. Smith +5

Understanding solar wind variability throughout the heliosphere is essential for fundamental space physics and future exploration of the Moon and Mars. The Mars Atmosphere and Vola…

astro-ph.SR2025

Properties of current sheets in two-dimensional tearing-mediated incompressible magnetohydrodynamic turbulence

Chen Shi, Marco Velli, Nikos Sioulas +1

It is well known that the nonlinear evolution of magnetohydrodynamic (MHD) turbulence generates current sheets. In the solar wind turbulence, current sheets are frequently observed…

astro-ph.SR2021★ 41 cited

Direct evidence for magnetic reconnection at the boundaries of magnetic switchbacks with Parker Solar Probe

C. Froment, V. Krasnoselskikh, T. Dudok de Wit +20

Parker Solar Probe's first encounters with the Sun revealed the presence of ubiquitous localised magnetic deflections in the inner heliosphere; these structures, often called switc…

astro-ph.SR2013★ 2 cited

Coupling the solar surface and the corona: coronal rotation, Alfvén wave-driven polar plumes

R. F. Pinto, R. Grappin, M. Velli +1

The dynamical response of the solar corona to surface and sub-surface perturbations depends on the chromospheric stratification, and specifically on how efficiently these layers re…

astro-ph.SR2009

Coupling Photosphere and Corona: Linear and Turbulent Regimes

A. Verdini, R. Grappin, M. Velli

In a recent work Grappin et al. [1] have shown that low- frequency movements can be transmitted from one footpoint to the other along a magnetic loop, thus mimicking a friction eff…