The properties of the solar corona and its connection to the solar wind
SR Cranmer, AR Winebarger - Annual Review of Astronomy …, 2019 - annualreviews.org
The corona is a layer of hot plasma that surrounds the Sun, traces out its complex magnetic
field, and ultimately expands into interplanetary space as the supersonic solar wind …
field, and ultimately expands into interplanetary space as the supersonic solar wind …
New view of the solar chromosphere
The solar chromosphere forms a crucial, yet complex and until recently poorly understood,
interface between the solar photosphere and the heliosphere.▪ Advances in high-resolution …
interface between the solar photosphere and the heliosphere.▪ Advances in high-resolution …
Hot explosions in the cool atmosphere of the Sun
The solar atmosphere was traditionally represented with a simple one-dimensional model.
Over the past few decades, this paradigm shifted for the chromosphere and corona that …
Over the past few decades, this paradigm shifted for the chromosphere and corona that …
Multi-scale variability of coronal loops set by thermal non-equilibrium and instability as a probe for coronal heating
Solar coronal loops are the building blocks of the solar corona. These dynamic structures
are shaped by the magnetic field that expands into the solar atmosphere. They can be …
are shaped by the magnetic field that expands into the solar atmosphere. They can be …
Probing the physics of the solar atmosphere with the Multi-slit Solar Explorer (MUSE). I. Coronal heating
Abstract The Multi-slit Solar Explorer (MUSE) is a proposed mission composed of a multislit
extreme ultraviolet (EUV) spectrograph (in three spectral bands around 171 Å, 284 Å, and …
extreme ultraviolet (EUV) spectrograph (in three spectral bands around 171 Å, 284 Å, and …
Dam** of slow magnetoacoustic oscillations by the misbalance between heating and cooling processes in the solar corona
Context. Rapidly decaying slow magnetoacoustic waves are regularly observed in the solar
coronal structures, offering a promising tool for a seismological diagnostics of the coronal …
coronal structures, offering a promising tool for a seismological diagnostics of the coronal …
Solar science with the Atacama Large Millimeter/Submillimeter Array—a new view of our Sun
Abstract The Atacama Large Millimeter/submillimeter Array (ALMA) is a new powerful tool for
observing the Sun at high spatial, temporal, and spectral resolution. These capabilities can …
observing the Sun at high spatial, temporal, and spectral resolution. These capabilities can …
Achievements of Hinode in the first eleven years
Hinode Review Team, K Al-Janabi… - Publications of the …, 2019 - academic.oup.com
Hinode is Japan's third solar mission following Hinotori (1981–1982) and Yohkoh (1991–
2001): it was launched on 2006 September 22 and is in operation currently. Hinode carries …
2001): it was launched on 2006 September 22 and is in operation currently. Hinode carries …
Are IRIS bombs connected to Ellerman bombs?
Recent observations by the Interface Region Imaging Spectrograph (IRIS) have revealed
pockets of hot gas (∼ 2–8× 10 4 K) potentially resulting from magnetic reconnection in the …
pockets of hot gas (∼ 2–8× 10 4 K) potentially resulting from magnetic reconnection in the …
Coronal rain in randomly heated arcades
Adopting the MPI-AMRVAC code, we present a 2.5-dimensional magnetohydrodynamic
simulation, which includes thermal conduction and radiative cooling, to investigate the …
simulation, which includes thermal conduction and radiative cooling, to investigate the …