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 …

In the following short review we will outline some of the possible interaction processes of
lower solar atmospheric plasma with the embedded small-scale solar magnetic fields. After …

Context. The atmospheres of cool main-sequence stars are structured by convective flows
from the convective envelope that penetrate the optically thin layers and lead to structuring …

Context. The Extreme Ultraviolet Imager (EUI) on board the Solar Orbiter (SO) spacecraft
observed small extreme ultraviolet (EUV) bursts, termed campfires, that have been proposed …

Context. The convective envelopes of cool main-sequence stars harbour magnetic fields
with a complex global and local structure. These fields affect the near-surface convection …

We report detection of oscillations in brightness temperature, size and horizontal velocity of
three small bright features in the chromosphere of a plage/enhanced-network region. The …

We present observations of transverse oscillations in slender Ca ii H fibrils (SCFs) in the
lower solar chromosphere. We use a 1 hr long time series of high-(spatial and temporal-) …

Bright points (BPs) in the solar photosphere are thought to be the radiative signatures (small-
scale brightness enhancements) of magnetic elements described by slender flux tubes or …

Aims. We used solar observations of a plage-enhanced network with the Atacama Large
Millimeter/sub-millimeter Array (ALMA) in Band 3 and Band 6, together with synthetic …

We characterize waves in small magnetic elements and investigate their propagation in the
lower solar atmosphere from observations at high spatial and temporal resolution. We use …