Some interesting topics provoked by the solar filament research in the past decade
Solar filaments are an intriguing phenomenon, like cool clouds suspended in the hot corona.
Similar structures exist in the intergalactic medium as well. Despite being a long-studied …
Similar structures exist in the intergalactic medium as well. Despite being a long-studied …
The solar upper transition region imager (SUTRI) onboard the SATech-01 satellite
Abstract The Solar Upper Transition Region Imager (SUTRI) onboard the Space Advanced
Technology demonstration satellite (SATech-01), which was launched to a Sun …
Technology demonstration satellite (SATech-01), which was launched to a Sun …
Application of a magnetic-field-induced transition in Fe X to solar and stellar coronal magnetic field measurements
Magnetic fields play a key role in driving a broad range of dynamic phenomena in the
atmospheres of the Sun and other stars. Routine and accurate measurements of the …
atmospheres of the Sun and other stars. Routine and accurate measurements of the …
Mapping the magnetic field in the solar corona through magnetoseismology
Magnetoseismology, a technique of magnetic field diagnostics based on observations of
magnetohydrodynamic (MHD) waves, has been widely used to estimate the field strengths …
magnetohydrodynamic (MHD) waves, has been widely used to estimate the field strengths …
Forward modeling of solar coronal magnetic-field measurements based on a magnetic-field-induced transition in Fe X
It was recently proposed that the intensity ratios of several extreme ultraviolet spectral lines
from Fe x ions can be used to measure the solar coronal magnetic field based on magnetic …
from Fe x ions can be used to measure the solar coronal magnetic field based on magnetic …
Toward a unified explanation for the three-part structure of solar coronal mass ejections
H Song, L Li, Y Chen - The Astrophysical Journal, 2022 - iopscience.iop.org
Coronal mass ejections (CMEs) are associated with the eruption of magnetic flux ropes
(MFRs), which usually appear as hot channels in active regions and coronal cavities in quiet …
(MFRs), which usually appear as hot channels in active regions and coronal cavities in quiet …
Solar coronal magnetic field measurements using spectral lines available in Hinode/EIS observations: strong and weak field techniques and temperature diagnostics
Recently, it has been proposed that the magnetic-field-induced transition (MIT) in Fe x can
be used to measure coronal magnetic field strengths. Several techniques, the direct line …
be used to measure coronal magnetic field strengths. Several techniques, the direct line …
The structure of coronal mass ejections recorded by the K-coronagraph at Mauna Loa solar observatory
Previous survey studies reported that coronal mass ejections (CMEs) can exhibit various
structures in white-light coronagraphs, and∼ 30% of them have the typical three-part feature …
structures in white-light coronagraphs, and∼ 30% of them have the typical three-part feature …
White-light coronal imaging at the 21 August 2017 total solar eclipse
JM Pasachoff, V Rušin - Solar Physics, 2022 - Springer
We describe the solar corona as imaged in the 21 August 2017 total solar eclipse from sites
in Oregon and Illinois, USA separated by nearly one hour. Our composite images, each …
in Oregon and Illinois, USA separated by nearly one hour. Our composite images, each …
A large-scale dataset of three-dimensional solar magnetic fields extrapolated by nonlinear force-free method
It has been widely accepted that solar magnetic field manipulates all solar activities,
especially violent solar bursts in solar corona. Thus, it is extremely important to reconstruct …
especially violent solar bursts in solar corona. Thus, it is extremely important to reconstruct …