Peter Barthol

TL;DR: The Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) as discussed by the authors is the scientific camera system onboard the Rosetta spacecraft, which consists of a high resolution Narrow Angle Camera (NAC) and a wide angle Camera (WAC) units accompanied by three electronics boxes.

TL;DR: The SUNRISE balloon-borne solar observatory consists of a 1 m aperture Gregory telescope, a UV filter imager, an imaging vector polarimeter, an image stabilization system, and further infrastructure as discussed by the authors.

TL;DR: The Imaging Magnetograph eXperiment (IMaX) is a spectropolarimeter built by four institutions in Spain that flew on board the Sunrise balloon-borne solar observatory in June 2009 for almost six days over the Arctic Circle as discussed by the authors.

TL;DR: The first science flight of the balloon-borne Sunrise telescope took place in June 2009 from ESRANGE (near Kiruna/Sweden) to Somerset Island in northern Canada.

TL;DR: The first science flight of the Sunrise balloon-borne solar observatory 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.