Magnetic reconnection in the era of exascale computing and multiscale experiments
Astrophysical plasmas have the remarkable ability to preserve magnetic topology, which
inevitably gives rise to the accumulation of magnetic energy within stressed regions …
inevitably gives rise to the accumulation of magnetic energy within stressed regions …
Magnetic reconnection: MHD theory and modelling
In this review we focus on the fundamental theory of magnetohydrodynamic reconnection,
together with applications to understanding a wide range of dynamic processes in the solar …
together with applications to understanding a wide range of dynamic processes in the solar …
Fast plasmoid-mediated reconnection in a solar flare
Magnetic reconnection is a multi-faceted process of energy conversion in astrophysical,
space and laboratory plasmas that operates at microscopic scales but has macroscopic …
space and laboratory plasmas that operates at microscopic scales but has macroscopic …
Transient small-scale brightenings in the quiet solar corona: A model for campfires observed with Solar Orbiter
Context. Recent observations by the Extreme Ultraviolet Imager (EUI) on board Solar Orbiter
have characterized prevalent small-scale transient brightenings in the corona above the …
have characterized prevalent small-scale transient brightenings in the corona above the …
Multi-scale variability of coronal loops set by thermal non-equilibrium and instability as a probe for coronal heating
Solar coronal loops are the building blocks of the solar corona. These dynamic structures
are shaped by the magnetic field that expands into the solar atmosphere. They can be …
are shaped by the magnetic field that expands into the solar atmosphere. They can be …
Probing the physics of the solar atmosphere with the multi-slit solar explorer (MUSE). II. flares and eruptions
MCM Cheung, J Martínez-Sykora, P Testa… - The Astrophysical …, 2022 - iopscience.iop.org
Current state-of-the-art spectrographs cannot resolve the fundamental spatial
(subarcseconds) and temporal (less than a few tens of seconds) scales of the coronal …
(subarcseconds) and temporal (less than a few tens of seconds) scales of the coronal …
Ultra-high-resolution observations of plasmoid-mediated magnetic reconnection in the deep solar atmosphere
LHMR van der Voort, M Van Noort… - Astronomy & …, 2023 - aanda.org
Context. Magnetic reconnection in the deep solar atmosphere can give rise to enhanced
emission in the Balmer hydrogen lines, a phenomenon referred to as Ellerman bombs. Aims …
emission in the Balmer hydrogen lines, a phenomenon referred to as Ellerman bombs. Aims …
Plasmoid instability in evolving current sheets and onset of fast reconnection
Plasmoid Instability in Evolving Current Sheets and Onset of Fast Reconnection - IOPscience
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Observations of turbulent magnetic reconnection within a solar current sheet
Magnetic reconnection is a fundamental physical process in various astrophysical, space,
and laboratory environments. Many pieces of evidence for magnetic reconnection have …
and laboratory environments. Many pieces of evidence for magnetic reconnection have …
The origin of reconnection-mediated transient brightenings in the solar transition region
SM Bahauddin, SJ Bradshaw, AR Winebarger - Nature Astronomy, 2021 - nature.com
The ultraviolet emission from the solar transition region is dominated by dynamic, low-lying
magnetic loops. The enhanced spatial and temporal resolution of the solar observation …
magnetic loops. The enhanced spatial and temporal resolution of the solar observation …