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 …
Magnetohydrodynamic oscillations in the solar corona and Earth's magnetosphere: towards consolidated understanding
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 …
Magnetohydrodynamic waves in open coronal structures
Modern observatories have revealed the ubiquitous presence of magnetohydrodynamic
waves in the solar corona. The propagating waves (in contrast to the standing waves) are …
waves in the solar corona. The propagating waves (in contrast to the standing waves) are …
Quasi-periodic energy release and jets at the base of solar coronal plumes
Coronal plumes are long, ray-like, open structures that have been considered as possible
sources of the solar wind. Their origin in the largely unipolar coronal holes has long been a …
sources of the solar wind. Their origin in the largely unipolar coronal holes has long been a …
Dispersion of slow magnetoacoustic waves in the active region fan loops introduced by thermal misbalance
SA Belov, NE Molevich, DI Zavershinskii - Solar Physics, 2021 - Springer
Slow magnetoacoustic waves observed in the solar corona are used as seismological
probes of plasma parameters. It has been shown that the dispersion properties of such …
probes of plasma parameters. It has been shown that the dispersion properties of such …
Acoustic Waves in a High-Temperature Plasma II. Dam** and Instability
BB Mikhalyaev, SB Derteev, NK Shividov… - Solar Physics, 2023 - Springer
In this article we study the properties of acoustic waves in the rarefied high-temperature
plasma of the solar corona, assuming that the heating and cooling of the plasma has a well …
plasma of the solar corona, assuming that the heating and cooling of the plasma has a well …
The effect of the magnetic field on the dam** of slow waves in the solar corona
TJ Duckenfield, DY Kolotkov… - Astronomy & Astrophysics, 2021 - aanda.org
Context. Slow magnetoacoustic waves are routinely observed in astrophysical plasma
systems such as the solar corona, and they are usually seen to damp rapidly. As a slow …
systems such as the solar corona, and they are usually seen to damp rapidly. As a slow …
Solar coronal magnetic fields derived using seismology techniques applied to omnipresent sunspot waves
DB Jess, VE Reznikova, RSI Ryans, DJ Christian… - Nature Physics, 2016 - nature.com
Sunspots on the surface of the Sun are the observational signatures of intense
manifestations of tightly packed magnetic field lines, with near-vertical field strengths …
manifestations of tightly packed magnetic field lines, with near-vertical field strengths …
Novel data analysis techniques in coronal seismology
We review novel data analysis techniques developed or adapted for the field of coronal
seismology. We focus on methods from the last ten years that were developed for extreme …
seismology. We focus on methods from the last ten years that were developed for extreme …
Mixed properties of slow magnetoacoustic and entropy waves in a plasma with heating/cooling misbalance
D Zavershinskii, D Kolotkov, D Riashchikov… - Solar Physics, 2021 - Springer
The processes of coronal plasma heating and cooling were previously shown to significantly
affect the dynamics of slow magnetoacoustic (MA) waves, causing amplification or …
affect the dynamics of slow magnetoacoustic (MA) waves, causing amplification or …