view article
Figure 3
(a) Simulated amplitude of the recorded time-resolved signal as a function of the sample thickness and of the XMCD contrast magnitude calculated according to equation (12)[link], and normalized to the optical density. The amplitude of the time-resolved signal is proportional to the magnitude of the XMCD contrast, γXMCD. (b) Same calculation as in (a), but utilizing the relation in equation (13)[link], normalized to ODexp(−OD). The results are effectively equal to the ones shown in (a), indicating that the first-order Taylor expansion is a reasonable approximation.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Volume 28| Part 4| July 2021| Pages 1146-1158
https://doi.org/10.1107/S1600577521004240
Follow J. Synchrotron Rad.
Sign up for e-alerts
E-alerts
Follow J. Synchrotron Rad. on Twitter
Twitter
Follow us on facebook
Facebook
Sign up for RSS feeds
RSS