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The Sunrise project is a balloon-borne solar observatory. It consists of a 1m aperture Gregory telescope, a UV filter imager, an imaging vector polarimeter, an image stabilization system and further infrastructure.
The SUNRISE project aims at high-resolution spectro-polarimetric observations of the solar atmosphere on the intrinsic spatial scale of its magnetic structure. The SUNRISE telescope with 1 m aperture and its instruments will provide spectra and images resolving spatial scales down to 35 km on the Sun. The main scientific goal of the mission is to understand the formation of magnetic structures in the solar atmosphere and to study their interaction with the convective plasma flows. The first science flight of Sunrise yielded high-quality data that reveal the structure, dynamics and evolution of solar convection, oscillations and magnetic fields at a resolution of around 100 km in the quiet Sun.
