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 …
Research progress based on observations of the New Vacuum Solar Telescope
XL Yan, Z Liu, J Zhang, Z Xu - Science China Technological Sciences, 2020 - Springer
The purpose of this paper is to introduce the main scientific results made by the one-meter
New Vacuum Solar Telescope (NVST), which was put into commission on 2010. NVST is …
New Vacuum Solar Telescope (NVST), which was put into commission on 2010. NVST is …
[PDF][PDF] Coronal EUV, QFP, and kink waves simultaneously launched during the course of jet–loop interaction
We present the observations of an extreme ultraviolet (EUV) wave, a quasi-periodic fast-
propagating (QFP) magnetosonic wave, and a kink wave that were simultaneously …
propagating (QFP) magnetosonic wave, and a kink wave that were simultaneously …
A fan spine jet: nonradial filament eruption and the plasmoid formation
H Li, J Yang - The Astrophysical Journal, 2019 - iopscience.iop.org
Using the data from SDO and NVST, we studied a circular filament eruption in association
with the formation of jet under a nonaxisymmetric fan spine configuration. A nonradial …
with the formation of jet under a nonaxisymmetric fan spine configuration. A nonradial …
Magnetic flux cancelation as the buildup and trigger mechanism for CME-producing eruptions in two small active regions
AC Sterling, RL Moore, NK Panesar - The Astrophysical Journal, 2018 - iopscience.iop.org
We follow two small, magnetically isolated coronal mass ejection (CME)-producing solar
active regions (ARs) from the time of their emergence until several days later, when their …
active regions (ARs) from the time of their emergence until several days later, when their …
Homologous large-amplitude nonlinear fast-mode magnetosonic waves driven by recurrent coronal jets
The detailed observational analysis of a homologous extreme-ultraviolet (EUV) wave event
is presented to study the driving mechanism and the physical property of the EUV waves …
is presented to study the driving mechanism and the physical property of the EUV waves …
The birth of a jet-driven twin CME and its deflection from remote magnetic fields
We report the formation of a complicated coronal mass ejection (CME) on 2015 August 23
by using the high temporal and high spatial resolution multi-wavelength observations taken …
by using the high temporal and high spatial resolution multi-wavelength observations taken …
An EUV jet driven by a series of transition region microjets
H Wei, Z Huang, H Fu, M Xiong, L Xia… - The Astrophysical …, 2022 - iopscience.iop.org
Jets are one of the most common eruptive events in the solar atmosphere, and they are
believed to be important in the context of coronal heating and solar wind acceleration. We …
believed to be important in the context of coronal heating and solar wind acceleration. We …
EUV waves driven by the sudden expansion of transequatorial loops caused by coronal jets
We present two events to study the driving mechanism of extreme-ultraviolet (EUV) waves
that are not associated with coronal mass ejections (CMEs), by using high-resolution …
that are not associated with coronal mass ejections (CMEs), by using high-resolution …
Dispersively formed quasi-periodic fast magnetosonic wavefronts due to the eruption of a nearby mini-filament
Observational analysis is performed to study the excitation mechanism and propagation
properties of a quasi-periodic fast-propagating (QFP) magnetosonic wave. The QFP wave …
properties of a quasi-periodic fast-propagating (QFP) magnetosonic wave. The QFP wave …