The Spectrometer Telescope for Imaging X-rays (STIX) is one of 10 instruments on board Solar Orbiter, a confirmed M- class mission of the European Space Agency (ESA) within the Cosmic Vision program scheduled to be launched in 2017. STIX applies a Fourier-imaging technique using a set of tungsten grids (at pitches from 0.038 to 1 mm) in front of 32 pixelized CdTe detectors to provide imaging spectroscopy of solar thermal and non-thermal hard X-ray emissions from 4 to 150 keV. The instrument passed the Preliminary Design Review (PDR) in early 2012.

Open PhD position

We have an open position for a PhD student in High Energy Heliophysics in collaboration with the Institute for Particle Physics at ETH. See the job-ad