Spectroscopic and spectropolarimetric measurements of the solar surface require high spatial and spectral resolution and special attention to instrument and data calibration. Our laboratory activity spans from the design and testing of imaging spectroscopy devices to the implementation and testing of novel approaches for Adaptive Optics. On top of this, we have a long-time expertise on data calibration pipelines.
The birth of Tor Vergata Fabry-Pérot interferometer
Optical cavity characterization of the Tor Vergata Fabry-Pérot interferometer
JP3D compression of solar data-cubes
The effects of AO systems on polarized light