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 …
A contemporary view of coronal heating
CE Parnell, I De Moortel - Philosophical Transactions of …, 2012 - royalsocietypublishing.org
Determining the heating mechanism (or mechanisms) that causes the outer atmosphere of
the Sun, and many other stars, to reach temperatures orders of magnitude higher than their …
the Sun, and many other stars, to reach temperatures orders of magnitude higher than their …
Wave heating of the solar atmosphere
I Arregui - … Transactions of the Royal Society A …, 2015 - royalsocietypublishing.org
Magnetic waves are a relevant component in the dynamics of the solar atmosphere. Their
significance has increased because of their potential as a remote diagnostic tool and their …
significance has increased because of their potential as a remote diagnostic tool and their …
Coronal heating by MHD waves
The heating of the solar chromosphere and corona to the observed high temperatures, imply
the presence of ongoing heating that balances the strong radiative and thermal conduction …
the presence of ongoing heating that balances the strong radiative and thermal conduction …
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 …
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 …
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 …
Magnetic Tornado Properties: A Substantial Contribution to the Solar Coronal Heating via Efficient Energy Transfer
In solving the solar coronal heating problem, it is crucial to comprehend the mechanisms by
which energy is conveyed from the photosphere to the corona. Recently, magnetic …
which energy is conveyed from the photosphere to the corona. Recently, magnetic …
Nonlinear propagation of Alfvén waves driven by observed photospheric motions: application to the coronal heating and spicule formation
T Matsumoto, K Shibata - The Astrophysical Journal, 2010 - iopscience.iop.org
We have performed MHD simulations of Alfvén wave propagation along an open flux tube in
the solar atmosphere. In our numerical model, Alfvén waves are generated by the …
the solar atmosphere. In our numerical model, Alfvén waves are generated by the …
Active region loops: Hinode/extreme-ultraviolet imaging spectrometer observations
We have carried out a study of active region loops using observations from the Extreme-
ultraviolet Imaging Spectrometer (EIS) on board Hinode using 1''raster data for an active …
ultraviolet Imaging Spectrometer (EIS) on board Hinode using 1''raster data for an active …