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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 …
Impact of space weather on climate and habitability of terrestrial-type exoplanets
The search for life in the Universe is a fundamental problem of astrobiology and modern
science. The current progress in the detection of terrestrial-type exoplanets has opened a …
science. The current progress in the detection of terrestrial-type exoplanets has opened a …
Wave heating of the solar atmosphere
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 …
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 …
High-frequency torsional Alfvén waves as an energy source for coronal heating
The existence of the Sun's hot atmosphere and the solar wind acceleration continues to be
an outstanding problem in solar-astrophysics. Although magnetohydrodynamic (MHD) …
an outstanding problem in solar-astrophysics. Although magnetohydrodynamic (MHD) …
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 …
Vortex motions in the solar atmosphere: Definitions, theory, observations, and modelling
Vortex flows, related to solar convective turbulent dynamics at granular scales and their
interplay with magnetic fields within intergranular lanes, occur abundantly on the solar …
interplay with magnetic fields within intergranular lanes, occur abundantly on the solar …
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 …