Author: Solarnet - High Resolution Solar Physics NetworkThe European Solar Telescope (EST) is of major interest for all the European Solar Community, since it will help to maintain Europe on the top of science, Solar Physics, and technology.
The EST design study was funded by the Eu ... more
Author: Vigeesh GangadharanTemperature perturbations in a magnetic flux sheet (strong field) due to waves excited by a horizontal motion at the bottom boundary. The excitation generates fast magneto-acoustic wave (predominantly magnetic) along with slow mag ... more
Author: Vigeesh GangadharanVariation of Stokes-V profiles of Fe I (5250.2 Å and 6302.5 Å) emerging from a small region on either side of the magnetic flux sheet (moderate field strength) as a result of wave propagation within the line-of-sight. The emerge ... more
Author: Klaus Gerhard PuschmannUpper panels from left to right: unsigned magnetic field strength; magnetic field inclination; magnetic Line-of-Sight velocity; magnetic field azimuth. Lower panels from left to right: Intensity; magnetic field polarity; Line-of-S ... more
Author: Klaus Gerhard PuschmannTime series VI (14 min). Left panel - reconstructed white-light intensity-maps @ 656nm. Right panel - Hα Line Wing intensities. Remarkable feature - interaction of small-scale quiet-sun magnetic field at solar disk center, driven ... more
Author: Christian NuttoThe sequence shows the evolution of dynamic structures resembling tornadoes in the solar atmosphere. The red lines represent stream lines of the velocity field in the solar atmosphere. The contour shows the dynamic evolution of th ... more
Author: Vigeesh GangadharanTemperature perturbations in a magnetic flux sheet (moderate field strength) due to waves excited by a horizontal motion at the bottom boundary. The waves higher up are predominantly acoustic (slow magneto-acoustic) that propagat ... more