A reconnection outflow in a simulated coronal MHD avalanche is identified and predicted to be measurable with MUSE but difficult with AIA.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Coronal energy release by MHD avalanches III. Identification of a reconnection outflow from a nanoflare
A reconnection outflow in a simulated coronal MHD avalanche is identified and predicted to be measurable with MUSE but difficult with AIA.