The 3rd harmonic Structure

Slides:



Advertisements
Similar presentations
EPS-HEP Aachen 2003R. Brinkmann, DESY Linear Colliders R. Brinkmann, DESY EPS-HEP Conference, Aachen, July 17, 2003.
Advertisements

The Continuing Role of SRF for AARD: Issues, Challenges and Benefits SRF performance has been rising every decade SRF installations for HEP (and other.
Areal RF Station A. Vardanyan RF System The AREAL RF system will consist of 3 RF stations: Each RF station has a 1 klystron, and HV modulator,
R&D For Accelerating Structures H. Padamsee. TESLA Niobium, one meter length, rf = 1.3 GHz Copper, 53 cm, rf = 11.4 GHz.
LEP3 RF System: gradient and power considerations Andy Butterworth BE/RF Thanks to R. Calaga, E. Ciapala.
Progress of ILC cavity gradient database and yield C.M. Ginsburg On behalf of the ILC Database Group Baseline Assessment Workshop, Tsukuba/WebEx September.
Latest Design of ILC ( RDR). 1.3 GHz technology developed by TESLA Collaboration, R&D from 1992 to reduce the cost per MeV by a factor of 20 from current.
1.3 GHz FNAL Dressed Cavity S-1 Global Deliverable to KEK 7 July 2009.
Accelerator R&D on LC - Activities of ATF & STF - 1. Introduction 2. ATF 3. STF 4. Summary Seiya Yamaguchi, KEK The US/Japan Collaboration in High Energy.
Rong-Li Geng Toward Higher Gradient and Q 0 LCWS2013, U. of TokyoNov , 2013, R.L. Geng1.
Cavity Yield Re-Evaluation Plan C.M. Ginsburg (Fermilab) July 10, 2009 (Essentially a copy of presentation June 24, 2009 to SCRF-ML WebEx meeting with.
F Status and Plans for SRF Facility Sergei Nagaitsev May 18, 2007.
ILC R&D at Fermilab Robert Kephart. ILC Americas f Fermilab May 15-18, 2006FY06 DOE Annual Review2 Outline Fermilab ILC Goals Fermilab’s role in the GDE.
The ILCTA_MDB Horizontal Test Stand for SRF Cavities Andy Hocker FNAL-TD AEM, 25-JUN-2007.
High Power RF Systems, Control and Distribution in the HINS Alfred Moretti, Brian Chase, Chris Jensen and Peter Prieto Fermilab Accelerator Advisory Committee.
TTF-II Status & Prospectives Nick Walker DESY 5 th ITRP Meeting – CALTECH.
XFEL SRF Accelerating Module Prototypes Tests at DESY Fermilab Seminar, July 21st Denis Kostin, MHF-SL, DESY.
Harmonics.
Nikolay SolyakILC-GDE, Beijing, Feb.4-8, Fermilab 3 rd Harmonic Cryomodule Status N.Solyak, H. Edwards, D.Mitchell, M.Foley, T.Khabiboulline, E.Harms,
Americas Region: T4CM Status and Plans H. Carter TD SRF Dev. Dept. July 14, 2006.
Designing of Learning Sequences Erik Engh QM Software.
Status of the International Linear Collider and Importance of Industrialization B Barish Fermilab 21-Sept-05.
Horizontal Test Stands and CC2 Results Andy Hocker Testing an alternative ILC cavity design at USPAS (Q 0 =2.23E+02)
Alors, c’est fini! Et maintenant?. Machine Upgrade in Stages Push LHC performance without new hardware –luminosity →2.3x10 34 cm -2 s -1, E b =7→7.54.
BCD input from WG2 WG2 12/08/2005 H. Hayano Chris Adolphsen Terry Garvey Hitoshi Hayano.
1Matthias LiepeAugust 2, 2007 Future Options Matthias Liepe.
Cavity Yield Re-Evaluation Plan C.M. Ginsburg (Fermilab) June 24, 2009.
Review 09/2010 page RF System for Electron Collider Ring Haipeng Wang for the team of R. Rimmer and F. Marhauser, SRF Institute and Y. Zhang, G. Krafft.
Ricarda Laasch | DESY Experiments on Thermal Cycling | 25th March 2014 | Page 1 Click to edit Master subtitle style Experiments on thermal cycling Measurements.
Progress and Plans for R&D and the Conceptual Design of the ILC Main Linacs H. Hayano, KEK PAC2005 5/18/2005.
@ Fermilab ILC bunch-compressor and linac rf requirements Sergei Nagaitsev Fermilab Feb. 9, 2006.
BEAMLINE HOM ABSORBER O. Nezhevenko, S. Nagaitsev, N. Solyak, V. Yakovlev Fermi National Laboratory December 11, 2007 Wake Fest 07 - ILC wakefield workshop.
Already time to think of upgrading the machine Two options presently discussed/studied Higher luminosity ~10 35 cm -2 s -1 (SLHC) –Needs changes in.
ILC Cryomodule Industrialization in the U.S. R. Kephart (+ H Padamsee )
Niobium RRR and Ta specifications for SRF cavities: a critical review G. Ciovati, P. Kneisel and G. Myneni 7 th SRF Materials Workshop, July 16 th 2012.
Start of S2 Milestone Work H. Padamsee. Intro At KEK S2 meeting we decided to make a list of milestones and eventually cost S2 activities I tried to start.
ILCTA-MDB RF Power Status 4/27/06 Reid 1 ILCTA-MDB Status 1.3 GHz RF Power 3.9 GHz RF Power Meson Detector Building April 27, 2006 [John Reid]
Optimization of FAST Electron Gun Beam Parameters Using ASTRA Lucas Kang Lee Teng Presentations August 6, 2015.
Experiments on thermal cycling
Field Emission Minimization for LCLS-II
Research Theme 2: Beam Acceleration (Superconducting RF Cavities)
Abstract EuSPARC and EuPRAXIA projects
Development of X-band 50MW klystron in BVERI
New Cavity Techniques and Future Prospects
E-XFEL Status and First Beam Results
X-band high-power variable RF splitter
for the FNAL/ANL, JLab, and Cornell cavity teams
S1-G cryomodule assembly status
The situation is far better than I had thought.
Status and Plan of GDE Design Work (Including Road Map for RDR)
Testing Infrastructure, Program and Milestones
R&D Activity for Field Emission and Vertical EP
Gu Qiang For the project team
2. SCRF General Preparation for the AD&I Preparation for AAP Review
WG 3 : Cavity Data Banks 9:00 ~ 10:30 Session-I 4 Talks
Progress in Asia Hitoshi Hayano,KEK,
Recent high-gradient testing results from the CLIC XBoxes
CW Operation of XFEL Modules
presented by Elmar Vogel
Degradation and possible sources Statistic of resonators
Summary on WG 2 LINAC Technology.
Collaboration Board Meeting Closing Hasan Padamsee
IHEP Cryomodule Status
Development of Large Grain Cavities at DESY
ESS Bilbao RF Systems Overview Pedro J. González
Status of RF at HZB: BESSY II, MLS, bERLinPro and BESSY VSR
FNAL update Martina Martinello.
Modified at -
Linearization of Bunch Compression (2nd order )
Novel Accelerator and Detector Systems
Presentation transcript:

The 3rd harmonic Structure Markus Hüning

Limitation by Physics According to BCS theory the surface resistance is approximately This limits the ultimate gradient which can be reached, At 1.3 GHz this number is 1 nW at 2 K, at 3.9 GHz it is 9 nW. The limit scales from 50 MV/m to 17 MV/m

Limitation cntd Limit at 3 GHz ~ 25 MV/m At Cornell 25 MV/m was reached (1400°C treatment) For 3.9 GHz this translates to

Reschke 94

Padamsee 93

Status at Fermilab

String

Status at DESY

Status at DESY Modulator being modified (parts available) Klystron expected in July Circulators overdue (Feb) Waveguides on the way