Kavli Affiliate: Ralf Heilmann | Summary:High-resolution ($R = λ/Δλ> 2000$) x-ray absorption and emission line spectroscopy in the soft x-ray band is a crucial diagnostic for the exploration of the properties of ubiquitous warm and hot plasmas and their dynamics in the cosmic web, galaxy clusters, galaxy halos, intragalactic space, and star atmospheres. Soft x-ray […]
Continue.. Toward volume manufacturing of high-performance soft x-ray critical-angle transmission gratings