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500 mA news : last update July 19, 2005SPEAR3 2004 Closeout ReportSPEAR3 Commissioning UpdateFirst SPEAR3 Beam
into SSRL Beam Line Hutch
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The next major milestone
for the SPEAR3 commissioning occurred at 17:56 on Monday, March
8, 2004, when the first SPEAR3 synchrotron light was observed
on a monitor located inside BL9-3's monochromator housing ![]() Fig. 2 |
![]() Fig. 1 |
A video which chronicles
the installation activities is available at:
http://www-ssrl.slac.stanford.edu/movies/spear3-oct-03.mpg
SSRL enters a new era of synchrotron radiation experimentation with the
completion of the SPEAR 3 upgrade project this Fall. The SPEAR 3 storage
ring, with parameters summarized in Table 1, produces beams having one
to two orders of magnitude higher brightness and flux density than the
old SPEAR 2 ring (Table 2), accommodates several new high performance
insertion devices and beam lines, and is capable of top-off operation
by virtue of its improved at-energy injection system. Brightness for
new undulators exceeds 1018 at 5 keV. The 4-year, 58 M$ upgrade project is administered by the DOE, with ~50% joint
funding from NIH.
The project has completely replaced the SPEAR vacuum chamber,
magnets, support rafts, RF, power supplies, cable plant and shielding
tunnel floor in a 7-month shutdown period that began March 31.
480 tons of SPEAR 2 magnet girders, vacuum chambers, power supplies,
and most cables and controls were removed from the SPEAR site. Shielding,
utilities and other ancillary systems were modified, a new cable plant
was installed in trays outside the tunnel, new power supplies were installed
in a refurbished building, a new concrete floor was poured and mounting
plates for SPEAR 3 magnet and vacuum chamber support girders were installed
and aligned. Pre-assembled girders were installed in the second week
of August, followed by straight section vacuum chamber, mode-damped
RF cavity, insertion device and beam line front end component installation
in September and early October. The vacuum system was be pumped down,
cable and utility connections completed, and the ring aligned in October.
System testing took place in November and beam commissioning is now
in progress. It is expected that beam will be available for users by
March of 2004.
SPEAR3 will operate at 100 mA for the first user run while beam line
optical components are upgraded and radiation shielding is added for
higher current operation. The accelerator physics and engineering groups
will fully utilize the first run to characterize and optimize ring lattice
and beam parameters, develop the fast orbit feedback system (having
a 4 kHz orbit acquisition rate), and to ascertain beam stability issues
that might be encountered at higher currents. Full 500-mA operation
is planned for the second user run beginning in the Fall of 2004.