Luca explaining the heat rejector prototype for the Gregor Telescope The students testing their Galileo replica telescopes Yesterday was a...
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An image of the moon captured tonight through the Newtonian telescope This week we also had our usual star party...
The first quarter of 2019 sees the exciting launch of one out of the five successfully retained INFRA-EOSC-04-2018 Cluster projects,...
On February 2nd 2017, Dr. Giorgio Viavattene presented his thesis entitled “Spectro-polarimetric analysis of a short lived solar active region" ...
ADAHELI+ :ADvanced Astronomy for HELIophysics Plus We present a study performed to address the ESA call for a small mission...
The overall diffusive motion of the selected magnetic elements. Their initial positions are rescaled to the origin. Here, delta x...
Flares and coronal mass ejections (CMEs) are solar phenomena that are not yet fully understood. Several investigations have been performed...
The long-term variability in stratospheric ozone mass mixing ratio (O3) and temperature (T) from 1979 to 2013 is investigated using...
Spectropolarimetry is nowadays one of the most used tool to investigate small scale (100 km) magnetic fields in the Sun’s...
The FORS (closed loop forecasting system) control algorithm has been already successfully applied to improve the efficiency of a simulated...
