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

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Showing astro-ph.SRShow all

5 papers · 1 filter

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…

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…