Waves in the lower solar atmosphere: the dawn of next-generation solar telescopes
Waves and oscillations have been observed in the Sun's atmosphere for over half a century.
While such phenomena have readily been observed across the entire electromagnetic …
While such phenomena have readily been observed across the entire electromagnetic …
Multiwavelength studies of MHD waves in the solar chromosphere: An overview of recent results
The chromosphere is a thin layer of the solar atmosphere that bridges the relatively cool
photosphere and the intensely heated transition region and corona. Compressible and …
photosphere and the intensely heated transition region and corona. Compressible and …
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 …
Transverse oscillations and an energy source in a strongly magnetized sunspot
D Yuan, L Fu, W Cao, B Kuźma, M Geeraerts… - Nature …, 2023 - nature.com
The solar corona is two to three orders of magnitude hotter than the underlying photosphere,
and the energy loss of coronal plasma is extremely strong, requiring a heating flux of over …
and the energy loss of coronal plasma is extremely strong, requiring a heating flux of over …
A statistical study of short-period decayless oscillations of coronal loops in an active region
Coronal loop oscillations are common phenomena in the solar corona, which are often
classified as decaying and decayless oscillations. Using the high-resolution observation …
classified as decaying and decayless oscillations. Using the high-resolution observation …
Magnetohydrodynamic fast sausage waves in the solar corona
Characterized by cyclic axisymmetric perturbations to both the magnetic and fluid
parameters, magnetohydrodynamic fast sausage modes (FSMs) have proven useful for …
parameters, magnetohydrodynamic fast sausage modes (FSMs) have proven useful for …
Resonant absorption of transverse oscillations and associated heating in a solar prominence. II. Numerical aspects
P Antolin, TJ Okamoto, B De Pontieu… - The Astrophysical …, 2015 - iopscience.iop.org
Transverse magnetohydrodynamic (MHD) waves are ubiquitous in the solar atmosphere
and may be responsible for generating the Sun's million-degree outer atmosphere …
and may be responsible for generating the Sun's million-degree outer atmosphere …
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 …
Investigating Alfvénic wave propagation in coronal open-field regions
The physical mechanisms behind accelerating solar and stellar winds are a long-standing
astrophysical mystery, although recent breakthroughs have come from models invoking the …
astrophysical mystery, although recent breakthroughs have come from models invoking the …