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Magnetohydrodynamic waves in the solar corona
The corona of the Sun is a unique environment in which magnetohydrodynamic (MHD)
waves, one of the fundamental processes of plasma astrophysics, are open to a direct study …
waves, one of the fundamental processes of plasma astrophysics, are open to a direct study …
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 …
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 …
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 …
Partially ionized plasmas in astrophysics
Partially ionized plasmas are found across the Universe in many different astrophysical
environments. They constitute an essential ingredient of the solar atmosphere, molecular …
environments. They constitute an essential ingredient of the solar atmosphere, molecular …
Alfvén wave dissipation in the solar chromosphere
Magnetohydrodynamic Alfvén waves have been a focus of laboratory plasma physics and
astrophysics for over half a century. Their unique nature makes them ideal energy …
astrophysics for over half a century. Their unique nature makes them ideal energy …
Probing the physics of the solar atmosphere with the multi-slit solar explorer (MUSE). II. flares and eruptions
Current state-of-the-art spectrographs cannot resolve the fundamental spatial
(subarcseconds) and temporal (less than a few tens of seconds) scales of the coronal …
(subarcseconds) and temporal (less than a few tens of seconds) scales of the coronal …
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 …
Alfvénic waves in the inhomogeneous solar atmosphere
The solar atmosphere is known to be replete with magneto-hydrodynamic wave modes, and
there has been significant investment in understanding how these waves propagate through …
there has been significant investment in understanding how these waves propagate through …
The european solar telescope
CQ Noda, R Schlichenmaier, LRB Rubio… - Astronomy & …, 2022 - aanda.org
The European Solar Telescope (EST) is a project aimed at studying the magnetic
connectivity of the solar atmosphere, from the deep photosphere to the upper …
connectivity of the solar atmosphere, from the deep photosphere to the upper …