view article

Figure 5
APU22 characteristics for the different harmonics in the energy range between 5.7 and 28 keV at the EMA and the MANACÁ beamlines at Sirius: (a) peak emission energy Eu as a function of the phase pu; (b) variation correlation between Eu and pu as a function of Eu; (c) energy tuning tolerance ratio as a function of pu; and (d) phase error tolerance [\Gamma_{p_{\rm{u}}}] as a function of pu.

Journal logoJOURNAL OF
SYNCHROTRON
RADIATION
ISSN: 1600-5775
Follow J. Synchrotron Rad.
Sign up for e-alerts
Follow J. Synchrotron Rad. on Twitter
Follow us on facebook
Sign up for RSS feeds