activity
20122026
most citedShear-Driven Transition to Isotropically Turbulent Solar Wind Outside the Alfven Critical Zone

126 citations · 252 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2026

Direct Measurement of Polar Coronal Hole-like Solar Wind in its Acceleration Phase

Samuel T. Badman, Yeimy J. Rivera, Michael L. Stevens +38

The early evolution of fast polar coronal hole (PCH) solar wind remains largely unconstrained by in situ measurements. In March 2025, Parker Solar Probe (Parker) at its closest app…

astro-ph.SR2026

Spherically Polarized Alfvén Waves and the Gosling Boost

Yuliang Ding, Marco Velli, Zesen Huang +6

Alfvén waves are thought to play critical roles in solar wind acceleration and plasma heating in the solar corona and inner heliosphere. Parker Solar Probe (PSP) has highlighted th…

astro-ph.SR2024

Applications of Fast Magnetic Reconnection Models to the Atmospheres of the Sun and Protoplanetary Disks

Fulvia Pucci, Alkendra Singh, Uma Gorti +4

Partially-ionized plasmas consist of charged and neutral particles whose mutual collisions modify magnetic reconnection compared with the fully-ionized case. The collisions alter t…

physics.space-ph2020★ 126 cited

Shear-Driven Transition to Isotropically Turbulent Solar Wind Outside the Alfven Critical Zone

D. Ruffolo, W. H. Matthaeus, R. Chhiber +11

Motivated by prior remote observations of a transition from striated solar coronal structures to more isotropic ``flocculated'' fluctuations, we propose that the dynamics of the in…

astro-ph.SR2019★ 10 cited

Magnetic field line twisting by photospheric vortices: energy storage and release

A. F. Rappazzo, M. Velli, R. B. Dahlburg +1

We investigate the dynamics of a closed corona cartesian reduced magnetohydrodynamic (MHD) model where photospheric vortices twist the coronal magnetic field lines. We consider two…

astro-ph.SR2015★ 53 cited

Observational Signatures of Coronal Loop Heating and Cooling Driven by Footpoint Shuffling

R. B. Dahlburg, G. Einaudi, B. D. Taylor +4

The evolution of a coronal loop is studied by means of numerical simulations of the fully compressible three-dimensional magnetohydrodynamic equations using the HYPERION code. The…

physics.plasm-ph2015★ 36 cited

"Ideal" tearing and the transition to fast reconnection in the weakly collisional MHD and EMHD regimes

Daniele Del Sarto, Fulvia Pucci, Anna Tenerani +1

This paper discusses the transition to fast growth of the tearing instability in thin current sheets in the collisionless limit where electron inertia drives the reconnection proce…

physics.space-ph2012★ 27 cited

Proton temperature anisotropy and magnetic reconnection in the solar wind: effects of kinetic instabilities on current sheet stability

Lorenzo Matteini, Simone Landi, Marco Velli +1

We investigate the role of kinetic instabilities driven by a proton anisotropy on the onset of magnetic reconnection by means of 2-D hybrid simulations. The collisionless tearing o…