Aims. The observation of propagating magneto-hydrodynamic kink waves in magnetic structures and measurement of their properties (amplitude, phase speed) can be used to diagnose the plasma conditions in the neighbourhood of the magnetic structure via magneto-seismology. We aim to reveal properties of the chromosphere/transition region above the sunspot penumbra using this technique. Methods. Hinode SOT observed a sunspot as it was crossing over the limb, providing a unique side on view of the atmosphere above a sunspot. The presence of large spicule-like jets is evident in Ca i
In recent years, new high spatial resolution observations of the Sun's atmosphere have revealed the ...
Since their discovery, spicules have attracted increased attention as energy/mass bridges between th...
Understanding the fine structures and transient phenomena associated with the origins of the fast so...
We use images of high spatial and temporal resolution, obtained using both ground- and space-based i...
We use images of high spatial and temporal resolution, obtained using both ground- and space-based i...
International audienceContext. For investigating spicules from the photosphere to coronal heights, t...
Context: The dynamic atmosphere of the Sun exhibits a wealth of magnetohydrodynamic (MHD) waves. In ...
Using data obtained by the high temporal and spatial resolution Rapid Oscillations in the Solar Atmo...
We use images of high spatial and temporal resolution, obtained with the Rapid Oscillations in the S...
International audienceSpicules are an important very dynamical and rather cool structure extending b...
Observations of jet- like phenomena near the solar limb are reported for a long time, firs...
Sunspots have played a key role in aiding our understanding of magnetohydrodynamic (MHD) wave phenom...
The chromosphere is a critical interface between the relatively cold photosphere and the hot corona....
The variation of magnetic field strength and plasma density along a solar spicule is determined by t...
Transverse magnetohydrodynamic waves often called Alfvénic (or kink) waves have been often theoretic...
In recent years, new high spatial resolution observations of the Sun's atmosphere have revealed the ...
Since their discovery, spicules have attracted increased attention as energy/mass bridges between th...
Understanding the fine structures and transient phenomena associated with the origins of the fast so...
We use images of high spatial and temporal resolution, obtained using both ground- and space-based i...
We use images of high spatial and temporal resolution, obtained using both ground- and space-based i...
International audienceContext. For investigating spicules from the photosphere to coronal heights, t...
Context: The dynamic atmosphere of the Sun exhibits a wealth of magnetohydrodynamic (MHD) waves. In ...
Using data obtained by the high temporal and spatial resolution Rapid Oscillations in the Solar Atmo...
We use images of high spatial and temporal resolution, obtained with the Rapid Oscillations in the S...
International audienceSpicules are an important very dynamical and rather cool structure extending b...
Observations of jet- like phenomena near the solar limb are reported for a long time, firs...
Sunspots have played a key role in aiding our understanding of magnetohydrodynamic (MHD) wave phenom...
The chromosphere is a critical interface between the relatively cold photosphere and the hot corona....
The variation of magnetic field strength and plasma density along a solar spicule is determined by t...
Transverse magnetohydrodynamic waves often called Alfvénic (or kink) waves have been often theoretic...
In recent years, new high spatial resolution observations of the Sun's atmosphere have revealed the ...
Since their discovery, spicules have attracted increased attention as energy/mass bridges between th...
Understanding the fine structures and transient phenomena associated with the origins of the fast so...