collaborators

9 papers

physics.space-ph2026

Reformation of Supercritical Perpendicular Shock

Yuri V. Khotyaintsev, Domenico Trotta, Daniel B. Graham

Super-critical collisionless shocks are not static structures but evolve continuously as they reflect incoming ions back upstream. The physical process responsible for this non-sta…

physics.space-ph2026

Energetic particle-mediated interplanetary shocks observed by Solar Orbiter

D. Trotta, D. Lario, B. Reville +10

Context: In collisionless shocks, energetic particles can carry sufficient pressure to modify the upstream plasma and the shock structure itself, a regime often invoked in theories…

astro-ph.SR2026

Energy Evolution from the Chromosphere to the Heliosphere in the 2021 October 28 Solar Eruption

Katharine K. Reeves, Daniel B. Seaton, Cynthia Cattell +20

We perform a detailed study of the energetics for a well-observed solar eruption and flare that occurred on 28 October 2021. This event included a GOES class X1.0 flare, a global E…

physics.space-ph2026

Compressive Structures in the Foreshock of Collisionless Shocks

Savvas Raptis, Domenico Trotta, Drew L. Turner +11

Collisionless shocks are fundamental accelerators of energetic particles; yet, the observations of nonlinear foreshock structures, which are essential in acceleration processes, di…

astro-ph.SR2025

Velocity-space turbulent cascade in the near-Sun solar wind: first insights from the Parker Solar Probe mission

A. Larosa, O. Pezzi, T. Bowen +11

In space plasmas, the rarity of collisions leads to complex structures in the velocity space where a turbulent cascade of the velocity distribution function fluctuations is thought…

physics.space-ph2025

Ion-Scale Solitary Structures in the Solar Wind Observed by Solar Orbiter and Parker Solar Probe

Yufei Yang, Timothy S. Horbury, Domenico Trotta +12

We investigate a class of ion-scale magnetic solitary structures in the solar wind, characterized by distinct magnetic field enhancements and bipolar rotations over spatial scales…