Observations of magnetic reconnection in the deep solar atmosphere in the Hε line
LHMR van der Voort, J Joshi, K Krikova - Astronomy & Astrophysics, 2024 - aanda.org
Context. Magnetic reconnection in the deep solar atmosphere can give rise to enhanced
emission in the Balmer hydrogen lines, a phenomenon known as Ellerman bombs (EBs). It …
emission in the Balmer hydrogen lines, a phenomenon known as Ellerman bombs (EBs). It …
Limb event brightenings and fast ejection using IRIS mission observations
Abstract The Interface Region Imaging Spectrograph (IRIS) of the recently commissioned
NASA small explorer mission provides significantly more complete and higher resolution …
NASA small explorer mission provides significantly more complete and higher resolution …
Properties and modeling of unresolved fine structure loops observed in the solar transition region by IRIS
Recent observations from the Interface Region Imaging Spectrograph (IRIS) have
discovered a new class of numerous low-lying dynamic loop structures, and it has been …
discovered a new class of numerous low-lying dynamic loop structures, and it has been …
Explosive events in active region observed by IRIS and SST/CRISP
Transition-region explosive events (EEs) are characterized by non-Gaussian line profiles
with enhanced wings at Doppler velocities of 50–150 km s− 1. They are believed to be the …
with enhanced wings at Doppler velocities of 50–150 km s− 1. They are believed to be the …
Signatures of ubiquitous magnetic reconnection in the lower solar atmosphere
J Joshi, LHMR van der Voort… - Astronomy & …, 2020 - aanda.org
Ellerman Bomb-like brightenings of the hydrogen Balmer line wings in the quiet Sun, also
known as quiet Sun Ellerman bombs (QSEBs), are a signature of the fundamental process of …
known as quiet Sun Ellerman bombs (QSEBs), are a signature of the fundamental process of …
Flare Ribbons Approach Observed by the Interface Region Imaging Spectrograph and the Solar Dynamics Observatory
T Li, J Zhang, Y Hou - The Astrophysical Journal, 2017 - iopscience.iop.org
We report flare ribbons approach (FRA) during a multiple-ribbon M-class flare on 2015
November 4 in NOAA AR 12443, obtained by the Interface Region Imaging Spectrograph …
November 4 in NOAA AR 12443, obtained by the Interface Region Imaging Spectrograph …
Bidirectional reconnection outflows in an active region
G Ruan, B Schmieder, S Masson, P Mein… - The Astrophysical …, 2019 - iopscience.iop.org
We report on bidirectional coronal reconnection outflows reaching±200 km s− 1 as observed
in an active region with the Si iv and C ii spectra of the Interface Region Imaging …
in an active region with the Si iv and C ii spectra of the Interface Region Imaging …
Signatures of quiet Sun reconnection events in Ca ii, Hα, and Fe i
We use observations of quiet Sun (QS) regions in the Hα 6563 Å, Ca ii 8542 Å, and Fe i
6302 Å lines. We observe brightenings in the wings of the Hα and Ca ii combined with …
6302 Å lines. We observe brightenings in the wings of the Hα and Ca ii combined with …
A magnetic reconnection event in the solar atmosphere driven by relaxation of a twisted arch filament system
We present high-resolution observations of a magnetic reconnection event in the solar
atmosphere taken with the New Vacuum Solar Telescope, Atmospheric Imaging Assembly …
atmosphere taken with the New Vacuum Solar Telescope, Atmospheric Imaging Assembly …
Observation of the Hall magnetic reconnection as close as 56 solar radii from the Sun
A few thin current layers were detected in the rear boundary of an interplanetary coronal
mass ejection (ICME) observed at 56 solar radii from the Sun as the Parker Solar Probe …
mass ejection (ICME) observed at 56 solar radii from the Sun as the Parker Solar Probe …