J. C. del Toro Iniesta

TL;DR: In this paper, an inversion code of Stokes line profiles is presented, which allows the recovery of the stratification of the temperature, the magnetic field vector, and the line of sight velocity through the atmosphere.

TL;DR: The first mission of ESA's Cosmic Vision 2015-2025 programme and a mission of international collaboration between ESA and NASA, was launched on 10 February 2020 04:03 UTC from Cape Canaveral and aims to address key questions of solar and heliospheric physics pertaining to how the Sun creates and controls the Heliosphere, and why solar activity changes with time.

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.