M. Herranz

TL;DR: In this article, the GIADA (Grain Impact Analyser and Dust Accumulator) experiment on the European Space Agency's Rosetta spacecraft orbiting comet 67P/Churyumov-Gerasimenko was used to detect 35 outflowing grains of mass 10−10 to 10−7 kilograms.

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 Imaging Magnetograph eXperiment (IMaX) is a spectropolarimeter built by four institutions in Spain that flew on board the Sunrise balloon-borne telesocope in June 2009 for almost six days over the Arctic Circle.

TL;DR: The grain impact analysis and dust accumulation (GIADA) instrument on board ESA's Rosetta mission is constraining the origin of the dust particles detected within the coma of comet 67 P/Churyumov-Gerasimenko (67P) as mentioned in this paper.

TL;DR: The Polarimetric and Helioseismic Imager on the Solar Orbiter mission (SO/PHI) as mentioned in this paper is the first magnetograph and helio-physics instrument to observe the Sun from outside the Sun-Earth line.