collaborators

6 papers

physics.plasm-ph2026

Numerical simulations of waves and turbulence in coronal loops: observables and spectra

Fabio Feraco, Francesco Pucci, Claudio Meringolo +11

We investigate numerically the time evolution of velocity and magnetic field fluctuations in a coronal loop, focusing on the dynamics due to both phase mixing and turbulent cascade…

astro-ph.SR2026

Anisotropic non-Maxwellian velocity distributions in the solar transition region

Paola Testa, Bart De Pontieu, Kyuhyoun Cho +1

High resolution spectral observations of transition region spectral lines capture the signatures of energy deposition and redistribution at the boundary between the lower and upper…

astro-ph.SR2026

On the cool nature of coronal nanojets

Gabriele Cozzo, Paola Testa, Juan Martinez-Sykora +5

Reconnection-driven nanoflares are widely considered a leading mechanism for coronal-loop heating, but their direct fingerprints in the tenuous coronal plasma remain elusive. The r…

astro-ph.SR2026

The connection between solar coronal abundances and the underlying lower atmospheric properties

Paola Testa, Juan Martinez-Sykora, Bart De Pontieu +4

Elemental abundances in the solar corona and solar wind are often observed to differ from those in the solar photosphere, most commonly showing an enhancement of low first ionizati…

astro-ph.SR2026

Multi-fluid multi-species models for inverse FIP-effect

Juan Martínez-Sykora, Paola Testa, Deborah Baker +1

The inverse First Ionization Potential (FIP) effect is rarely observed in the solar atmosphere, and this anomaly poses a challenging problem in understanding physical processes dri…

astro-ph.SR2025

Solar Flare Ion Temperatures

Alexander J. B. Russell, Vanessa Polito, Paola Testa +2

This paper proposes that the ion temperature is several times the local electron temperature in the hot onset phase and at the above-the-loop region of solar flares. The paper cons…