X-Ray Storage Ring
Introduction & History
The
X-ray ring at the National Synchrotron Light Source
was one of the first storage rings designed as a dedicated source of synchrotron
radiation. The final lattice design was completed in 1978 shortly after funding
was approved. Construction started in FY 1979 and installation of the magnets
was well underway by the end of FY 1981. The first stored beam was obtained in
September 1982. By FY 1985 the experimental program was in a rapid state of
development, and by the end of FY 1990 the Phase II beamlines and insertion
devices were being brought into operation. Implementation of global
orbit feedback systems stabilized the orbit for all users, and local
orbit feedback provided enhanced stability for the insertion device beamlines. In
Spring 1993, a current of 500 ma was stored at 2.5 GeV. Also the vertical
emittance was reduced by a factor of six down to below 2 Angstroms, corresponding to a horizontal-vertical
coupling of 0.002. In 1996 operating current was increased to 350 mA at 2.584 GeV. In period of 1999-2000
X-ray ring has had alternating operations between high emittance lattice at 2.800GeV and low emittance lattice
at 2.584 GeV. In August 2000 the ring started regular operations with low emmitance lattice at 300 mA, 2.800GeV.
The increase of energy together with the reduction of vertical emittance yields an order of magnitude increase in brightness.
The lattice design for the X-ray ring is an eight
superperiod Green-Chasman or double bend achromatic lattice with a circumference of ~ 170 meters. The
achromatic bend is comprised of two 22.5 degree dipole bending magnets and a single focusing quadrupole. The
dispersion free insertion straight sections are bounded by quadrupole triplets. The beta functions at the
insertion center are quite small, betax = 1.5 m and betay = 0.33 m, resulting in very small transverse beam
dimensions, but somewhat larger angular spread. Some advantages of low beta insertions are: the effect of the
wiggler magnetic fields on the lattice are minimized, the brightness is optimized for short high- field wigglers,
and the low vertical beta function allows the development of very
small gap devices
situated at the insertion center. An important disadvantage of low beta insertions is that orbit variations can
result in large vertical angular deviations which could illuminate uncooled portions of the vacuum chamber with high
power wiggler radiation. For this reason it has been necessary to develop special active interlock systems which use
pick-up electrodes on either end of the straight section to detect orbit motion and to dump the electron beam if
orbit movements are too large.