Coronal loops: observations and modeling of confined plasma
F Reale - Living Reviews in Solar Physics, 2014 - Springer
Coronal loops are the building blocks of the X-ray bright solar corona. They owe their
brightness to the dense confined plasma, and this review focuses on loops mostly as …
brightness to the dense confined plasma, and this review focuses on loops mostly as …
On solving the coronal heating problem
JA Klimchuk - Solar Physics, 2006 - Springer
The question of what heats the solar corona remains one of the most important problems in
astrophysics. Finding a definitive solution involves a number of challenging steps, beginning …
astrophysics. Finding a definitive solution involves a number of challenging steps, beginning …
[HTML][HTML] The solar orbiter mission-science overview
D Müller, OCS Cyr, I Zouganelis, HR Gilbert… - Astronomy & …, 2020 - aanda.org
Aims. Solar Orbiter, the first mission of ESA's Cosmic Vision 2015–2025 programme and a
mission of international collaboration between ESA and NASA, will explore the Sun and …
mission of international collaboration between ESA and NASA, will explore the Sun and …
Physics of solar prominences: II—magnetic structure and dynamics
DH Mackay, JT Karpen, JL Ballester, B Schmieder… - Space Science …, 2010 - Springer
Observations and models of solar prominences are reviewed. We focus on non-eruptive
prominences, and describe recent progress in four areas of prominence research:(1) …
prominences, and describe recent progress in four areas of prominence research:(1) …
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 …
Thermal instability and non-equilibrium in solar coronal loops: from coronal rain to long-period intensity pulsations
P Antolin - Plasma Physics and Controlled Fusion, 2019 - iopscience.iop.org
The complex interaction of the magnetic field with matter is the key to some of the most
puzzling observed phenomena at multiple scales across the Universe, from tokamak plasma …
puzzling observed phenomena at multiple scales across the Universe, from tokamak plasma …
Observing the fine structure of loops through high-resolution spectroscopic observations of coronal rain with the CRISP instrument at the Swedish Solar Telescope
P Antolin, LR van Der Voort - The Astrophysical Journal, 2012 - iopscience.iop.org
Observed in cool chromospheric lines, such as Hα or Ca ii H, coronal rain corresponds to
cool and dense plasma falling from coronal heights. Considered as a peculiar sporadic …
cool and dense plasma falling from coronal heights. Considered as a peculiar sporadic …
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 …
Sensitivity of detachment extent to magnetic configuration and external parameters
Divertor detachment may be essential to reduce heat loads to magnetic fusion tokamak
reactor divertor surfaces. Yet in experiments it is difficult to control the extent of the detached …
reactor divertor surfaces. Yet in experiments it is difficult to control the extent of the detached …