activity
20022026
most citedSolar Coronal Jets: Observations, Theory, and Modeling

361 citations · 1.9k across the 37 of their papers we have counts for

collaborators

37 papers

astro-ph.SR2026

Current Sheet Fragmentation in the Course of Repeated Eruptive Magnetic Flux Emergence

Vaggelis Karantanis, Loukas Vlahos, Heinz Isliker +2

Magnetic reconnection between emerging magnetic flux and the ambient coronal field fundamentally drives solar jets. We use three-dimensional resistive-MHD simulations of eruptive f…

astro-ph.SR2025

Observations of microwave emission from solar jets and comparison with MHD simulations

Costas E. Alissandrakis, Vasilis Archontis, Kostas Moraitis

We computed the thermal microwave emission from a 3D magnetohydrodynamic (MHD) simulation and compared it with observations of solar jets. The simulation treats the emergence of ma…

astro-ph.SR2025

Magnetic flux cancellation in a flux-emergence magnetohydrodynamics simulation of coronal hole eruptions and jets

Spiros Patsourakos, Vasilis Archontis

We search for signatures of magnetic flux cancellation in a 3D resistive MHD flux-emergence simulation of coronal jets and eruptions in a coronal-hole-like environment. To do this,…

astro-ph.SR2025

Recurrent eruptions from the emergence of a toroidal flux tube

J. Zhuleku, V. Archontis, K. Moraitis

Solar eruptive behavior is often modeled with magnetohydrodynamic simulations of magnetic flux emergence. The usual geometry considered is that of a horizontal cylindrical magnetic…

astro-ph.SR2024

Magnetic flux emergence and solar eruptions in partially ionized plasmas

Georgios Chouliaras, V. Archontis

We have performed 3D MHD simulations to study the effect of partial ionization in the process of magnetic flux emergence in the Sun. In fact, we continue previous work and we now f…

astro-ph.SR2024

Magnetic helicity and energy budgets of jet events from an emerging solar active region

A. Nindos, S. Patsourakos, K. Moraitis +4

Using photospheric vector magnetograms obtained by the Helioseismic and Magnetic Imager on board the Solar Dynamics Observatory and a magnetic connectivity-based method, we compute…