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 …
Quasi-periodic pulsations in solar flares
VM Nakariakov, VF Melnikov - Space Science Reviews, 2009 - Springer
Quasi-periodic pulsations (QPP) are a common feature of flaring energy releases in the
solar atmosphere, observed in all bands, from radio to hard X-ray. In this review we …
solar atmosphere, observed in all bands, from radio to hard X-ray. In this review we …
[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 …
Magnetohydrodynamic oscillations in the solar corona and Earth's magnetosphere: towards consolidated understanding
VM Nakariakov, V Pilipenko, B Heilig, P Jelínek… - Space Science …, 2016 - Springer
Magnetohydrodynamic (MHD) oscillatory processes in different plasma systems, such as the
corona of the Sun and the Earth's magnetosphere, show interesting similarities and …
corona of the Sun and the Earth's magnetosphere, show interesting similarities and …
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 …
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 …
Modelling quasi-periodic pulsations in solar and stellar flares
JA McLaughlin, VM Nakariakov, M Dominique… - Space Science …, 2018 - Springer
Solar flare emission is detected in all EM bands and variations in flux density of solar
energetic particles. Often the EM radiation generated in solar and stellar flares shows a …
energetic particles. Often the EM radiation generated in solar and stellar flares shows a …
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 …
Spatial and Temporal Analysis of Quiescent Coronal Rain over an Active Region
The solar corona produces coronal rain, hundreds of times colder and denser material than
the surroundings. Coronal rain is known to be deeply linked to coronal heating, but its origin …
the surroundings. Coronal rain is known to be deeply linked to coronal heating, but its origin …
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 …