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Studies with carbon coatings in the SPS - MD run, week 25

Studies with carbon coatings in the SPS - MD run, week 25

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<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand Futureplans<strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC30 June 2009<strong>SPS</strong>U-team (G.Ardu<strong>in</strong>i, F.Caspers, S. Calatroni, P. Chiggiato,K. Cornelis, B. Henrist, E. Mahner, E. Metral, G. Rumolo, E.Shaposhnikova, M. Taborelli, F. Zimmermann), P. Costa P<strong>in</strong>to,E. BenedettoChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand Futureplans1 Overview of <strong>SPS</strong> <strong>MD</strong> <strong>run</strong>s2 Overview of <strong>carbon</strong> coated l<strong>in</strong>ers <strong>in</strong>serted <strong>in</strong> <strong>SPS</strong>3 Overview of <strong>carbon</strong> coated magnets <strong>in</strong>serted <strong>in</strong> <strong>SPS</strong>4 Conclusions and Future plansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


<strong>SPS</strong> scrubb<strong>in</strong>g <strong>run</strong><strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansMonday 15/6 (18:00) - Tuesday 16/6 (05:00) : 1-3batches <strong>with</strong> 48 bunchesTuesday 16/6 (19:00) - Wednesday 17/6 (10:00): 2-3batches <strong>with</strong> 72 bunchesThursday 17/6 (00:00) - Thursday 18/6 (08:30): 2-3batches <strong>with</strong> 72 bunches, <strong>with</strong> accelerationThe nom<strong>in</strong>al LHC cycle of 21.6 s.Christ<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


L<strong>in</strong>ers used for E-cloud monitor<strong>in</strong>g<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand Futureplans1 Sta<strong>in</strong>less Steel (ref): SEMCLOUD1, channel 1-48, XSD12 a-C stripe (width: 40mm): SEMCLOUD1, channel 49-96,SDneg3 a-C on Zr (rough surface): SEMCLOUD2, channel 1-48,EcEx4 a-C (CNe13, been <strong>in</strong> <strong>SPS</strong> s<strong>in</strong>ce last year): SEMCLOUD2,channel 49-96, XSD2All <strong>the</strong> tests were done <strong>in</strong> <strong>the</strong> magnets at a field of 1.2kGauss.The beam energy <strong>in</strong> <strong>the</strong> scrubb<strong>in</strong>g <strong>run</strong> was 450 GeV/cChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Carbon Coat<strong>in</strong>gs<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>a-C stripe/CNe32 - width 40 mmChrist<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Carbon Coat<strong>in</strong>gs<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>a-C/Zr: CNeZr <strong>run</strong> 10 Rough surface.a-C: CNe13, been <strong>in</strong> <strong>SPS</strong> s<strong>in</strong>ce last year.Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Results from FBCT<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Results from <strong>the</strong> E-cloud monitors<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Schematic draw<strong>in</strong>g of <strong>the</strong> magnets<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Pressure read<strong>in</strong>g before <strong>the</strong> <strong>MD</strong> <strong>run</strong> (Background pressure).The pressure between <strong>the</strong> two coated magnet is twice higherthan <strong>the</strong> one between <strong>the</strong> uncoated magnets.Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Pressure read<strong>in</strong>g - Before <strong>the</strong> scrubb<strong>in</strong>g <strong>run</strong><strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Pressure read<strong>in</strong>g - Maximum of <strong>the</strong> pressures<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Pressure read<strong>in</strong>g - Maximum of <strong>the</strong> pressures<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Conclusions<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Scrubb<strong>in</strong>g Run: StStδ max = 2.<strong>25</strong>, higher than δ threshold = 1.3Normalized E-Cloud Current/FBCT started at -0.35, <strong>the</strong>same as from <strong>the</strong> previous <strong>run</strong>.After 3 nights scrubb<strong>in</strong>g, E-Cloud has been reduced bynearly 30%.Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Conclusions<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Scrubb<strong>in</strong>g Run: StStδ max = 2.<strong>25</strong>, higher than δ threshold = 1.3Normalized E-Cloud Current/FBCT started at -0.35, <strong>the</strong>same as from <strong>the</strong> previous <strong>run</strong>.After 3 nights scrubb<strong>in</strong>g, E-Cloud has been reduced bynearly 30%.Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Conclusions<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Scrubb<strong>in</strong>g Run: StStδ max = 2.<strong>25</strong>, higher than δ threshold = 1.3Normalized E-Cloud Current/FBCT started at -0.35, <strong>the</strong>same as from <strong>the</strong> previous <strong>run</strong>.After 3 nights scrubb<strong>in</strong>g, E-Cloud has been reduced bynearly 30%.Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Conclusions<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Scrubb<strong>in</strong>g Run: a-C stripδ max = 0.92, lower than δ threshold = 1.3IT WORKS! BUT, <strong>the</strong> width of 40mm is a bit too low.It gives 350 times lower E-Cloud compared to StSt.After 3 nights scrubb<strong>in</strong>g, E-Cloud has been reduced bynearly a factor of 2.Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Conclusions<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Scrubb<strong>in</strong>g Run: a-C stripδ max = 0.92, lower than δ threshold = 1.3IT WORKS! BUT, <strong>the</strong> width of 40mm is a bit too low.It gives 350 times lower E-Cloud compared to StSt.After 3 nights scrubb<strong>in</strong>g, E-Cloud has been reduced bynearly a factor of 2.Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Conclusions<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Scrubb<strong>in</strong>g Run: a-C stripδ max = 0.92, lower than δ threshold = 1.3IT WORKS! BUT, <strong>the</strong> width of 40mm is a bit too low.It gives 350 times lower E-Cloud compared to StSt.After 3 nights scrubb<strong>in</strong>g, E-Cloud has been reduced bynearly a factor of 2.Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Conclusions<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Scrubb<strong>in</strong>g Run: a-C stripδ max = 0.92, lower than δ threshold = 1.3IT WORKS! BUT, <strong>the</strong> width of 40mm is a bit too low.It gives 350 times lower E-Cloud compared to StSt.After 3 nights scrubb<strong>in</strong>g, E-Cloud has been reduced bynearly a factor of 2.Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Conclusions<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Scrubb<strong>in</strong>g Run: a-C on Zrδ max = 0.96, lower than δ threshold = 1.3It started at <strong>the</strong> same level as a-C strip.After 3 nights scrubb<strong>in</strong>g, E-Cloud has been reduced bynearly a factor of 10.Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Conclusions<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Scrubb<strong>in</strong>g Run: a-C on Zrδ max = 0.96, lower than δ threshold = 1.3It started at <strong>the</strong> same level as a-C strip.After 3 nights scrubb<strong>in</strong>g, E-Cloud has been reduced bynearly a factor of 10.Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Conclusions<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Scrubb<strong>in</strong>g Run: a-C on Zrδ max = 0.96, lower than δ threshold = 1.3It started at <strong>the</strong> same level as a-C strip.After 3 nights scrubb<strong>in</strong>g, E-Cloud has been reduced bynearly a factor of 10.Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Conclusions<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Scrubb<strong>in</strong>g Run: a-C CNe13Initial δ max = 1.0Has been <strong>in</strong> <strong>the</strong> <strong>SPS</strong> s<strong>in</strong>ce last year. It gives 4 times lowere-cloud from <strong>the</strong> start than <strong>the</strong> new <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong>.After 3 nights scrubb<strong>in</strong>g, almost no E-Cloud effect can bedetected.Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Conclusions<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Scrubb<strong>in</strong>g Run: a-C CNe13Initial δ max = 1.0Has been <strong>in</strong> <strong>the</strong> <strong>SPS</strong> s<strong>in</strong>ce last year. It gives 4 times lowere-cloud from <strong>the</strong> start than <strong>the</strong> new <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong>.After 3 nights scrubb<strong>in</strong>g, almost no E-Cloud effect can bedetected.Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Conclusions<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Scrubb<strong>in</strong>g Run: a-C CNe13Initial δ max = 1.0Has been <strong>in</strong> <strong>the</strong> <strong>SPS</strong> s<strong>in</strong>ce last year. It gives 4 times lowere-cloud from <strong>the</strong> start than <strong>the</strong> new <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong>.After 3 nights scrubb<strong>in</strong>g, almost no E-Cloud effect can bedetected.Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Conclusions<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansPressure read<strong>in</strong>g <strong>in</strong> <strong>the</strong> magnetsBefore <strong>the</strong> <strong>in</strong>jection of <strong>the</strong> beam, <strong>the</strong> background pressurebetween <strong>the</strong> coated magnets was 2 times higher than <strong>the</strong>pressure between uncoated magnets. ⇒ Due to <strong>the</strong> higheroutgass<strong>in</strong>g <strong>in</strong> <strong>the</strong> <strong>carbon</strong> film and shorter pump<strong>in</strong>g time.With acceleration, <strong>the</strong> pressure between <strong>the</strong> coatedmagnets became as high as <strong>the</strong> pressure between <strong>the</strong>uncoated magnets.The gauges for measur<strong>in</strong>g <strong>the</strong> pressure between twocoated magnets are close to a quadrupole. ⇐ Highdegass<strong>in</strong>g <strong>in</strong> <strong>the</strong> quadrupole? Not really comparable <strong>with</strong><strong>the</strong> gauge we took between <strong>the</strong> two uncoated magnets.Christ<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Conclusions<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansPressure read<strong>in</strong>g <strong>in</strong> <strong>the</strong> magnetsBefore <strong>the</strong> <strong>in</strong>jection of <strong>the</strong> beam, <strong>the</strong> background pressurebetween <strong>the</strong> coated magnets was 2 times higher than <strong>the</strong>pressure between uncoated magnets. ⇒ Due to <strong>the</strong> higheroutgass<strong>in</strong>g <strong>in</strong> <strong>the</strong> <strong>carbon</strong> film and shorter pump<strong>in</strong>g time.With acceleration, <strong>the</strong> pressure between <strong>the</strong> coatedmagnets became as high as <strong>the</strong> pressure between <strong>the</strong>uncoated magnets.The gauges for measur<strong>in</strong>g <strong>the</strong> pressure between twocoated magnets are close to a quadrupole. ⇐ Highdegass<strong>in</strong>g <strong>in</strong> <strong>the</strong> quadrupole? Not really comparable <strong>with</strong><strong>the</strong> gauge we took between <strong>the</strong> two uncoated magnets.Christ<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Conclusions<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansPressure read<strong>in</strong>g <strong>in</strong> <strong>the</strong> magnetsBefore <strong>the</strong> <strong>in</strong>jection of <strong>the</strong> beam, <strong>the</strong> background pressurebetween <strong>the</strong> coated magnets was 2 times higher than <strong>the</strong>pressure between uncoated magnets. ⇒ Due to <strong>the</strong> higheroutgass<strong>in</strong>g <strong>in</strong> <strong>the</strong> <strong>carbon</strong> film and shorter pump<strong>in</strong>g time.With acceleration, <strong>the</strong> pressure between <strong>the</strong> coatedmagnets became as high as <strong>the</strong> pressure between <strong>the</strong>uncoated magnets.The gauges for measur<strong>in</strong>g <strong>the</strong> pressure between twocoated magnets are close to a quadrupole. ⇐ Highdegass<strong>in</strong>g <strong>in</strong> <strong>the</strong> quadrupole? Not really comparable <strong>with</strong><strong>the</strong> gauge we took between <strong>the</strong> two uncoated magnets.Christ<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sOverview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Plans for <strong>the</strong> next <strong>MD</strong>1 Read <strong>the</strong> pressure close to l<strong>in</strong>ers2 F<strong>in</strong>d a gauge between two uncoated magnets close to aquadrupole.Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>


Thanks<strong>Studies</strong> <strong>with</strong><strong>carbon</strong><strong>coat<strong>in</strong>gs</strong> <strong>in</strong><strong>the</strong> <strong>SPS</strong>- <strong>MD</strong> <strong>run</strong>,<strong>week</strong> <strong>25</strong>Christ<strong>in</strong>a Y<strong>in</strong>VallgrenTE-VSCOutl<strong>in</strong>eOverview of<strong>SPS</strong> <strong>MD</strong> <strong>run</strong>sThanks a lot for your attention!Questions???Overview of<strong>carbon</strong> coatedl<strong>in</strong>ers <strong>in</strong>serted<strong>in</strong> <strong>SPS</strong>Overview of<strong>carbon</strong> coatedmagnets<strong>in</strong>serted <strong>in</strong><strong>SPS</strong>Conclusionsand FutureplansChrist<strong>in</strong>a Y<strong>in</strong> VallgrenTE-VSC <strong>Studies</strong> <strong>with</strong> <strong>carbon</strong> <strong>coat<strong>in</strong>gs</strong> <strong>in</strong> <strong>the</strong> <strong>SPS</strong> - <strong>MD</strong> <strong>run</strong>, <strong>week</strong> <strong>25</strong>

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