Title: Injector PP Setup Plan and Status
1Injector PP Setup Plan and Status
Haixin Huang
November 18, 2008
2Sources of Polarization Loss
- Category the known polarization loss into three
parts - Overall loss due to the horizontal resonances
with real ramp rate. (related to horizontal
emit.) - Near injection due to vertical tune outside spin
tune gap. (related to vertical tune and emit. ) - Loss due to snake resonances, mostly near 36?y .
(related to vertical emit.) - There may still be some additional polarization
loss due to not perfect vertical tune path or too
large a tune spread.
3Strategy to Overcome Polarization Loss
- There are significant emittance growth in the
injector chain - Emittance growth in the LEBT/MEBT of linac.
- Multiple scattering at stripping foil at LtB.
- BtA optics mismatch.
- The plan is to solve these emittance growth
problem one by one - LEBT/MEBT upgrade (currently under testing)
- Change the LtB foil manipulate beta function at
the foil to reduce the emittance growth (Will
test it after Jan. 12) - BtA study to better understand the BtA line and
AGS optical model. (data analysis underway) - Setup AGS injection with vertical tune in the
spin tune gap (gt8.95). (Working on the modeling) - Installation of two tune jump quads to mitigate
the polarization loss due to horizontal
resonances. - Change RF setup from h12 to h6 to reduce space
charge effect (more important due to expected
smaller emittances).
4LEBT/MEBT Upgrade Status
(from Deepak)
- OPPIS source was reconfigured and tested. OPPIS
source is fully operational - High intensity source being reassembled and
tested - LEBT (35 KeV) line for both sources are built and
under vacuum - Beam from OPPIS was transport to RFQ and
transmission (from OPPIS to the end of RFQ) is as
expected (gt90 for OPPIS solenoid off, 65 for
OPPIS solenoid on) - We are putting one more EINZEL lens (contingency
plan) to provide one more degree of freedom to
match into the RFQ. - MEBT (75 KeV) line was vacuum tested, and found
RFQ was 2 mm lower than Tank-1 - Now, we are realigning MEBT.
- We plan to put beam (both, polarized and high
intensity) in Tank -1 in the 1st week of Dec. - On schedule to be ready by early Jan.
5Horizontal Tune Jump Status
- Ceramic chambers have been ordered.
- Cables pulling is going on (which is a must
before run starts). - Control hardware purchase has started.
- P/S will be modified from existing ones. Some
parts have been ordered. - Magnet coil and assembly have started bidding
process. - Expect to get the magnets around end of Jan. They
will be tested by magnet division. - Current schedule is that the magnets can be
installed sometime in early March during
maintenance day. We would like to have 3-4 weeks
time to commission them.
6AGS Setup
- Start Booster on Jan. 12. With LEBT/MEBT upgrade,
it is worthwhile to check the emittances at the
BtA. The new LtB foil test and the beta function
manipulation at LtB foil will be the major work. - Start the three weeks of setup time before blue
ready for beam Jan. 19 - CSNK 2.1T WSNK 1.53T as usual.
- AGS RF setup same as last year (h12), we may
switch to h6 when RHIC is up running (due to
limited resources from RF group for RHIC LLRF
upgrade). - Apply the knowledge gained from BtA studies to
get a matched optics. - Injection optics injection with dwell field but
high vertical tune (gt8.95). It is worth of trying
to see if it is feasible. - Horizontal tune will set close to 8.70 throughout
the ramp to make tune jump setup easier. - Horizontal tune jump wont be ready on day one.
The gain on polarization is hoped from smaller
emittance out of linac and better matching at AGS
injection.
7Backup Slides
8Run6 Polarization vs. Intensity
model
fitting
Experimental data are normalized to the 200MeV
polarization and then assuming 82 AGS input.
Model prediction taken into account AGS input as
82, spin mismatch at injection and C15. The
emittance dependence on intensity was taken from
fitting of measurements between 3/21/06-6/12/06
?x9.212.30I ?y 7.904.13I, where I is
intensity in unit of 1011.
9Spin Tune and Qy vs Gg
(Courtesy of Nick)