activity
19982026
most citedTwo-scale structure of the electron dissipation region during collisionless magnetic reconnection

321 citations · 4.7k across the 94 of their papers we have counts for

collaborators

95 papers

astro-ph.SR2026

A New Framework for Modeling Solar Flares from MHD to Kinetic Processes

Joel C. Allred, Graham S. Kerr, Silvina E. Guidoni +4

Physical processes in solar flares span many orders of magnitude in spatiotemporal scales, so a single unified model accounting for all relevant processes remains computationally i…

astro-ph.SR2026

Plasma Heating and Energization in Hot-Onset Flare Precursor Events

H. Da, J. F. Drake, M. Swisdak

Recent observations of solar flares have revealed a distinct 'hot onset' phase preceding the impulsive phase, characterized by elevated plasma temperature (>10 MK), a steady increa…

astro-ph.SR2026

Solar-Cycle Modulation and Photospheric Magnetic Control of Turbulence in the Young Solar Wind

Yanwen Wang, Rohit Chhiber, Arcadi V. Usmanov +2

The solar wind is an outflow of solar plasma that expands from the corona to fill the heliosphere. Its turbulence provides a pathway for non-adiabatic heating and acceleration, and…

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…

astro-ph.SR2026

Signatures of Reconnection and a Split Heliospheric Tail in High-Energy Energetic Neutral Atoms

M. Kornbleuth, M. Opher, J. F. Drake +10

The shape of the heliosphere, regarded as comet-like since the 1960s, has recently been the subject of intense debate in the last decade. There is disagreement whether the heliosph…

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…