Context. The study of stellar activity is important because it can provide new constraints for dynamo models when combined with surface rotation rates and the...
Magnetic activity of red giants: Correlation between the amplitude of solar-like oscillations and chromospheric indicators
Previous studies have found that red giants (RGs) in close binary systems undergoing spin-orbit resonance exhibit an enhanced level of magnetic activity with...
Magnetic cycles and rotation periods of late-type stars from photometric time series
Aims: We investigate the photometric modulation induced by magnetic activity cycles and study the relationship between rotation period and activity cycle(s) in...
Magnetic field amplification and structure formation by the Rayleigh-Taylor instability
We report our results from a set of high-resolution, two-fluid, non-linear simulations of the magnetized Rayleigh Taylor instability (RTI) at the interface...
Magnetic field diagnostics of prominences with the Mg II k line 3D Stokes inversions versus traditional methods
The Mg II k resonance line is commonly used for diagnosing the solar chromosphere. We theoretically investigated its intensity and polarization in solar...
Magnetic field emergence in mesogranular-sized exploding granules observed with sunrise/IMaX data
We report on magnetic field emergences covering significant areas of exploding granules. The balloon-borne mission Sunrise provided high spatial and temporal...
Aims:We describe a new form of small-scale magnetic flux emergence in the quiet Sun. This process seems to take vertical magnetic fields from subsurface layers...
Magnetic field fluctuations in the shocked umbral chromosphere
Context. Umbral chromospheric observations show the presence of magnetoacoustic shocks. Several recent studies have reported magnetic field fluctuations...