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Open AccessPolarisation of decayless kink oscillations of solar coronal loops
Decayless kink oscillations of plasma loops in the solar corona may contain an answer to the enigmatic problem of solar and stellar coronal heating. The polarisation of the oscillations gives us a unique infor...
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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 ultraviolet (EUV) imaging observat...
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Open AccessA New View of the Solar Interface Region from the Interface Region Imaging Spectrograph (IRIS)
The Interface Region Imaging Spectrograph (IRIS) has been obtaining near- and far-ultraviolet images and spectra of the solar atmosphere since July 2013. IRIS is the highest resolution observatory to provide seam...
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Open AccessCritical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)
The National Science Foundation’s Daniel K. Inouye Solar Telescope (DKIST) will revolutionize our ability to measure, understand, and model the basic physical processes that control the structure and dynamics of ...
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Publisher Correction: Reconnection nanojets in the solar corona
An amendment to this paper has been published and can be accessed via a link at the top of the paper.
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Reconnection nanojets in the solar corona
The solar corona is shaped and mysteriously heated to millions of degrees by the Sun’s magnetic field. It has long been hypothesized that the heating results from a myriad of tiny magnetic energy outbursts cal...
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Coronal Heating by MHD Waves
The heating of the solar chromosphere and corona to the observed high temperatures, imply the presence of ongoing heating that balances the strong radiative and thermal conduction losses expected in the solar ...
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Article
Temporal and Spatial Scales in Coronal Rain Revealed by UV Imaging and Spectroscopic Observations
Coronal rain corresponds to cool and dense clumps in the corona accreting towards the solar surface; it is often observed above solar active regions. These clumps are generally thought to be produced by a ther...
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Article
On-Disk Coronal Rain
Small and elongated, cool and dense blob-like structures are being reported with high resolution telescopes in physically different regions throughout the solar atmosphere. Their detection and the understandin...
