Solar coronal jets: observations, theory, and modeling
NE Raouafi, S Patsourakos, E Pariat, PR Young… - Space Science …, 2016 - Springer
Coronal jets represent important manifestations of ubiquitous solar transients, which may be
the source of significant mass and energy input to the upper solar atmosphere and the solar …
the source of significant mass and energy input to the upper solar atmosphere and the solar …
Probable detection of an eruptive filament from a superflare on a solar-type star
K Namekata, H Maehara, S Honda, Y Notsu… - Nature …, 2022 - nature.com
Solar flares are often accompanied by filament/prominence eruptions (~ 104 K and~ 1010−
11 cm− 3), sometimes leading to coronal mass ejections that directly affect the Earth's …
11 cm− 3), sometimes leading to coronal mass ejections that directly affect the Earth's …
Observation and modelling of solar jets
Y Shen - Proceedings of the Royal Society A, 2021 - royalsocietypublishing.org
The solar atmosphere is full of complicated transients manifesting the reconfiguration of the
solar magnetic field and plasma. Solar jets represent collimated, beam-like plasma …
solar magnetic field and plasma. Solar jets represent collimated, beam-like plasma …
On a coronal blowout jet: the first observation of a simultaneously produced bubble-like CME and a jet-like CME in a solar event
The coronal blowout jet is a peculiar category among various jet phenomena, in which the
sheared base arch, often carrying a small filament, experiences a miniature version of …
sheared base arch, often carrying a small filament, experiences a miniature version of …
Three-dimensional modeling of quasi-homologous solar jets
E Pariat, SK Antiochos, CR DeVore - The Astrophysical Journal, 2010 - iopscience.iop.org
Recent solar observations (eg, obtained with Hinode and STEREO) have revealed that
coronal jets are a more frequent phenomenon than previously believed. This higher …
coronal jets are a more frequent phenomenon than previously believed. This higher …
On a solar blowout jet: driving mechanism and the formation of cool and hot components
Y Shen, YD Liu, J Su, Z Qu, Z Tian - The Astrophysical Journal, 2017 - iopscience.iop.org
We present observations of a blowout jet that experienced two distinct ejection stages. The
first stage started from the emergence of a small positive magnetic polarity, which was …
first stage started from the emergence of a small positive magnetic polarity, which was …
The Hα surges and EUV jets from magnetic flux emergences and cancellations
YC Jiang, HD Chen, KJ Li, YD Shen… - Astronomy & …, 2007 - aanda.org
We analyzed multi-wavelength observations of three surges with a recurrent period of about
70 min in H α, EUV, and soft X-ray, which occurred in the quiet-sun region on 2000 …
70 min in H α, EUV, and soft X-ray, which occurred in the quiet-sun region on 2000 …
Multiwavelength observations of small-scale reconnection events triggered by magnetic flux emergence in the solar atmosphere
SL Guglielmino, LRB Rubio, F Zuccarello… - The Astrophysical …, 2010 - iopscience.iop.org
The interaction between emerging magnetic flux and the pre-existing ambient field has
become a" hot" topic for both numerical simulations and high-resolution observations of the …
become a" hot" topic for both numerical simulations and high-resolution observations of the …
Blobs in recurring extreme-ultraviolet jets
QM Zhang, HS Ji - Astronomy & Astrophysics, 2014 - aanda.org
Context. Coronal jets are one type of ubiquitous small-scale activity that is caused by
magnetic reconnection in the solar corona. They are often associated with cool surges in the …
magnetic reconnection in the solar corona. They are often associated with cool surges in the …
Recurrent solar jets induced by a satellite spot and moving magnetic features
Recurrent and homologous jets were observed to the west edge of active region NOAA
11513 at the boundary of a coronal hole. We find two kinds of cancellations between …
11513 at the boundary of a coronal hole. We find two kinds of cancellations between …