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Magnetohydrodynamic waves and coronal seismology: an overview of recent results
Recent observations have revealed that magnetohydrodynamic (MHD) waves and
oscillations are ubiquitous in the solar atmosphere, with a wide range of periods. We give a …
oscillations are ubiquitous in the solar atmosphere, with a wide range of periods. We give a …
Flare-productive active regions
Strong solar flares and coronal mass ejections, here defined not only as the bursts of
electromagnetic radiation but as the entire process in which magnetic energy is released …
electromagnetic radiation but as the entire process in which magnetic energy is released …
Prevalence of small-scale jets from the networks of the solar transition region and chromosphere
As the interface between the Sun's photosphere and corona, the chromosphere and
transition region play a key role in the formation and acceleration of the solar wind …
transition region play a key role in the formation and acceleration of the solar wind …
Quasi-periodic pulsations in solar flares
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] Flux emergence (theory)
Magnetic flux emergence from the solar convection zone into the overlying atmosphere is
the driver of a diverse range of phenomena associated with solar activity. In this article, we …
the driver of a diverse range of phenomena associated with solar activity. In this article, we …
Probing the physics of the solar atmosphere with the Multi-slit Solar Explorer (MUSE). I. Coronal heating
Abstract The Multi-slit Solar Explorer (MUSE) is a proposed mission composed of a multislit
extreme ultraviolet (EUV) spectrograph (in three spectral bands around 171 Å, 284 Å, and …
extreme ultraviolet (EUV) spectrograph (in three spectral bands around 171 Å, 284 Å, and …
Plasma jets and eruptions in solar coronal holes: a three-dimensional flux emergence experiment
ABSTRACT A three-dimensional (3D) numerical experiment of the launching of a hot and
fast coronal jet followed by several violent eruptions is analyzed in detail. These events are …
fast coronal jet followed by several violent eruptions is analyzed in detail. These events are …
Modelling quasi-periodic pulsations in solar and stellar flares
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 …
Above-the-loop-top oscillation and quasi-periodic coronal wave generation in solar flares
Observations revealed that various kinds of oscillations are excited in solar flare regions.
Quasi-periodic pulsations (QPPs) in flare emissions are commonly observed in a wide range …
Quasi-periodic pulsations (QPPs) in flare emissions are commonly observed in a wide range …
Quasi-periodic pulsations in solar and stellar flares: an overview of recent results (invited review)
Quasi-periodic pulsations (or QPPs) are periodic intensity variations in the flare emission
that occur across all wavelength bands. In this article, we review the observational and …
that occur across all wavelength bands. In this article, we review the observational and …