The high brilliance EXAFS CDR proposes to convert one branch of the energy dispersive XAS beamline ID24 to a scanning EXAFS beamline to provide optimal conditions for Time-resolved and Extreme conditions XAS. This will allow to fully exploit the 40-fold decrease in source size offered by EBS. It will provide a 0.5x0.5 microns^2 (FWHM) spot for XAS/XES spectroscopy in a large energy range from 5-40 KeV, expanding the capacity of the ESRF spectroscopy beamline portfolio towards studies of highly dilute systems at extreme conditions and/or in a time resolution.

Scientific spokesperson:
Carlo Lamberti, University of Torino, Torino, Italy

Expert panel:
Max Wilke; University of Potsdam, Potsdam, Germany
Per Anders Carlsson; Chalmers University of Technology, Göteborg, Sweden
Paola D'Angelo; University of Roma, Roma, Italy
Manuel Munoz; University of Montpellier II, Montpellier, France

SAC observer:
Giacomo Ghiringhelli; Politecnico di Milano, Milano, Italy

ESRF coordinators:
Olivier Mathon; ESRF, BM23
Sakura Pascarelli; ESRF, ID24

Registration to this workshop is closed; Programme of this workshop

Contact: ebs-science