Proper motions in a sunspot group with a δ-configuration and close to the solar disk center have been studied by employing local correlation tracking techniques...
On the nature of kink MHD waves in magnetic flux tubes
Context: Magnetohydrodynamic (MHD) waves are often reported in the solar atmosphere and usually classified as slow, fast, or Alfvén. The possibility that these...
On the origin of magnetic driven winds and the structure of the galactic dynamo in isolated galaxies
We investigate the build-up of the galactic dynamo and subsequently the origin of a magnetic driven outflow. We use a set-up of an isolated disc galaxy with a...
On the origin of reverse polarity patches found by Hinode in sunspot penumbrae
Context: The topology of penumbral magnetic fields is poorly known. The satellite Hinode has recently revealed penumbral structures of a magnetic polarity that...
On the period ratio P1/2P2 in the oscillations of coronal loops
Aims.With strong evidence of fast and slow magnetoacoustic modes arising in the solar atmosphere there is scope for improved determinations of coronal...
On the Probable Existence of an Abrupt Magnetization in the Upper Chromosphere of the Quiet Sun
We report on a detailed radiative transfer modeling of the observed scattering polarization in the Hα line, which allows us to infer quantitative information on...
On the Robustness of the Pendulum Model for Large-amplitude Longitudinal Oscillations in Prominences
Large-amplitude longitudinal oscillations (LALOs) in prominences are spectacular manifestations of solar activity. In such events nearby energetic disturbances...
On the Scaling of the Damping Time for Resonantly Damped Oscillations in Coronal Loops
There is not as yet full agreement on the mechanism that causes the rapid damping of the oscillations observed by TRACE in coronal loops. It has been suggested...
On the sensitivity of the Halpha scattering polarization to chromospheric magnetism
A particularly interesting line for exploring the physical conditions of the quiet solar chromosphere is Halpha , but its intensity profile is magnetically...