Synchrotron light or radiation is part of the electromagnetic spectrum emitted by electrons when accelerated at relativistic speeds. At ALBA, we generate this type of light by accelerating electrons up to almost the speed of light (99,999%).
To know more about how we producte this light, check the Accelerators section. This synchrotron light arrives at the beamlines, where scientists bring the samples they want to analyse. When synchrotron light interacts with the sample, scientists obtain very precise and useful information, not available with other analytical tools.