10.10.2000J.Wenninger - LEP fest1 Energy Calibration at LEP Spins, Tides Vagabond Currents J. WenningerLEP fest 10.10.2000 and.

Slides:



Advertisements
Similar presentations
Chapter 11 S3 Tides. Ch 11 S3 Essential Questions 1. What causes tides? 2. What affects the heights of tides? 3. How are tides a source of energy?
Advertisements

The Preassembling Installation Survey & Alignment Accelerator Center of IHEP Qu Huamin 2006 / 4 / 27.
AIM: How do interactions among objects in space and their forces affect objects and cause predictable & regular changes on Earth? 5/1/13 DO NOW: Pick.
Beam energy calibration: systematic uncertainties M. Koratzinos FCC-ee (TLEP) Physics Workshop (TLEP8) 28 October 2014.
MONALISA: Interferometric Position Monitor at the Nanometre Scale David Urner Paul Coe Matthew Warden Armin Reichold Oxford University.
Tides - The Last Wave Information by the University of California (Riverside) updated in 2014.
Tides.
1 Tides We experience tides on Earth when the ocean level rises and falls. We experience 2 high tides and 2 low tides in a little over one day. But what.
The sun, the moon and the earth. 2. The Effect of the Sun and the Moon on the Earth.
Solar System Physics Astronomy 311 Professor Lee Carkner Lecture 6.
LIGO-G W Commissioning Data on Vibration Isolation & Suspensions Fred Raab 24 October 02.
K. Moffeit 6 Jan 2005 WORKSHOP Machine-Detector Interface at the International Linear Collider SLAC January 6-8, 2005 Polarimetry at the ILC Design issues.
Beam Dynamics Tutorial, L. Rivkin, EPFL & PSI, Prague, September 2014 Synchrotron radiation in LHC: spectrum and dynamics The Large Hadron Collider (LHC)
WIN'05, June A. Klier - Muon Collider Physics1 Physics at a Future Muon Collider Amit Klier University of California, Riverside WIN’05 – Delphi,
Solar System Physics Astronomy 311 Professor Lee Carkner Lecture 6.
Tides. What is a tide TIDE: A periodic short-term change in the height of the ocean surface at a particular place. A tide is one huge _______________.
Tides are periodic rises and falls of large bodies of water. Tides are caused by the gravitational pull of the moon and inertia. Most coastal areas see.
Explaining Earth’s Position & Motion in the Universe
STRIPLINE KICKER STATUS. PRESENTATION OUTLINE 1.Design of a stripline kicker for beam injection in DAFNE storage rings. 2.HV tests and RF measurements.
08/06/ FCC-ee with kinks Can we conserve polarized beams?
Section 7.3 Learning Goals: I will understand key terms: rotation, revolution, tilt, solstice, eclipse I will understand how Earth’s tilt affect the season.
KICKER LNF David Alesini LNF fast kickers study group* * D. Alesini, F. Marcellini P. Raimondi, S. Guiducci.
___________________ Jürgen Schreiber, ECFA/DESY LC workshop, Amsterdam, April 1-4, 2003 BEAM ENERGY SPECTROMETER DESY – Dubna – TU Berlin Machine physicists,
Status of the Beamline Simulation A.Somov Jefferson Lab Collaboration Meeting, May 11, 2010.
Polarimetry of Proton Beams at RHIC A.Bazilevsky Summer Students Lectures June 17, 2010.
Midterm 1 Review Please swipe your student ID for attendance tracking, and pick up your assigned transmitter.
1 Status of EMMA Shinji Machida CCLRC/RAL/ASTeC 23 April, ffag/machida_ ppt & pdf.
Earth’s Movement RotationRevolution  The spinning of an object around an axis. Example: - The Earth completes a full rotation in 24 hours  The movement.
1 BROOKHAVEN SCIENCE ASSOCIATES Abstract Magnet and Girder Integration Lewis Doom, NSLS-II Project National Synchrotron Light Source II (NSLS-II) will.
Thomas Roser Snowmass 2001 June 30 - July 21, 2001 Polarized Proton Acceleration and Collisions Spin dynamics and Siberian Snakes Polarized proton acceleration.
Energy calibration at LHC J. Wenninger. Motivation In general there is not much interest for accurate knowledge of the momentum in hadron machines. 
1 Options for low energy spin manipulation Ken Moffeit, SLAC 2009 Linear Collider Workshop of the Americas 29 September to 3 October 2009 K. Moffeit, D.
Plans for Polarized Beams at VEPP-2000 and U-70 Yu.Shatunov BINP, Novosibirsk P S IN 2006.
#1 Energy matching It is observed that the orbit of an injected proton beam is horizontally displaced towards the outside of the ring, by about  x~1 mm.
AIM: How does gravity affect the movement of planets?
08/06/ Beam Polarization at FCC-ee. 2 Transverse polarization both in the Z resonance region : 44 to 47 GeV beam energy, around half integer spin.
Spin Injection June 5, 2015 APEX Meeting H. Huang, P. Oddo, V. Ptitsyn.
LHC Beam Energy 1 J. Wenninger CERN Beams Department Operation group / LHC.
Essential Question: What causes tides in the oceans?
Motion of the Earth, the Moon and PlanetsEarthMoonPlanets.
J-PARC Spin Physics Workshop1 Polarized Proton Acceleration in J-PARC M. Bai Brookhaven National Laboratory.
Earth, Moon & Sun Seasons & Tides. Essential Standards 6.E.1Understand the earth/moon/sun system, and the properties, structures and predictable motions.
Ken Moffeit SLAC LCWA09 1 Polarization Considerations for CLIC Ken Moffeit, SLAC 2009 Linear Collider Workshop of the Americas 29 September to 3 October.
Principals of fast injection and extraction R. Apsimon.
Electron Spectrometer: Status July 14 Simon Jolly, Lawrence Deacon 1 st July 2014.
First results from CMD-3 detector at VEPP-2000 collider Budker Institute of Nuclear Physics, SB RAS, Novosibirsk, Russia September 2011 E.Solodov (for.
About polarized protons acceleration at U-70 A.Otboyev, P.Shatunov, Yu.Shatunov BINP, Novosibirsk S.Ivanov, S.Nurushev IHEP, Protvino Dubna Spin-05.
Transverse polarization for energy calibration at Z-peak M. Koratzinos With valuable input from Alain Blondel ICFA HF2014, Sunday, 12/10/2014.
Thomas Roser SPIN 2006 October 3, 2006 A Study of Polarized Proton Acceleration in J-PARC A.U.Luccio, M.Bai, T.Roser Brookhaven National Laboratory, Upton,
Status of RHIC Polarization Studies. Summary of Polarization Studies during Run09 Tune scans: – Nearby 0.7 – Near integer tune Polarization ramp measurement.
1 LHC Beam Energy J. Wenninger CERN Beams Department Operation group / LHC Acknowledgments: E. Todesco.
P. Chevtsov for the ELIC Design Team
Earth from a million miles
J.Wenninger - Mini-Workshop on Stray Fields
Energy calibration issues for FCC-ee I. Koop, BINP, Novosibirsk
THE SUN-MOON-EARTH SYSTEM
Accelerating and injecting polarized beams into FCC-ee I
High precision measurement of the beam energy at VEPP-4M collider by Yury Tikhonov KEDR&VEPP-4M collaboration Budker INP, Novosibirsk Outlook Introduction.
Longitudinal Diagnostics for start-up
Earth, Moon & Sun Seasons & Tides.
The Motions of Earth & the Moon.
Motions of Earth, The Moon and Planets
Energy Calibration of the SPS with Proton and Lead Ion Beams
Unit 8 Vocabulary Axis – imaginary line about which an object rotates
Electroweak bosons  .
electric dipole moments (EDM)
Things that happen on Earth
Spin Transparency Study and Test
Energy Calibration at LEP3 Lessons of LEP(2) 4 LEP3
Progress Update on the Electron Polarization Study in the JLEIC
Presentation transcript:

J.Wenninger - LEP fest1 Energy Calibration at LEP Spins, Tides Vagabond Currents J. WenningerLEP fest and

J.Wenninger - LEP fest2 Polarization at LEP Under the influence of synchrotron radiation, the LEP beams polarize spontaneously (align their spins) in the transverse (vertical) direction. Polarization is a slow and delicate process which requires a lot of care and special machine conditions ! record P T = 57% routine P T = 5 -10% At LEP : Ideal machine : P T max = 92.4% Up to 60.6 GeV

J.Wenninger - LEP fest3 Resonant Depolarization The number of precessions/turn is proportional to the energy : Resonant depolarization To determine the energy Measure ! Principle :  Get a fast magnet (“kicker”).  Sweep the B-field and observe P T.  If kicker frequency and match, P T is rotated away from the vertical axis. The interest of P T : magnetic moments precess in B-fields.

J.Wenninger - LEP fest4 In the control room :Intrinsic accuracy :  E < 0.4 MeV  E/E <  E < 0.4 MeV  E/E < Resonant Depolarization II  Sweep the magnet frequency over a selected interval (~ 22 Hz).  Observe the effect on P T. This is more than one order of magnitude better than any other method ! But it requires an large amount of DEDICATED beam time !

J.Wenninger - LEP fest5 Z Resonance Scans Good regions for P T are ~ 50 MeV wide and spaced by 441 MeV. Convenient for Z mass and width measurements ! Calibrations cannot be performed during “physics” (no P T with colliding beams) Beam energy model Extrapolation in time

J.Wenninger - LEP fest6 Stressed Rings Sensitivity of the energy to circumference changes : At LEP resonant depolarization is sensitive to circumference changes of  C/C ~ ! At LEP resonant depolarization is sensitive to circumference changes of  C/C ~ ! 1991 : the first calibrations revealed unexplained fluctuations of the beam energy. A SLAC ground motion expert suggested… tides ! The beam samples different fields.

J.Wenninger - LEP fest7 Earth Tides Tide bulge of a celestial body of mass M at a distance d :  = angle(vertical,the celestial body) Earth tides :  The Moon contributes 2/3, the Sun 1/3.  NO 12 hour symmetry (direction of Earth rotation axis).  Not resonance-driven (unlike Sea tides !).  Accurate predictions.

J.Wenninger - LEP fest8 Moonrise over LEP Fall of 1992 : The historic tide experiment !  The total strain is 4 x (  C = 1 mm)

J.Wenninger - LEP fest9 Success in the Press !

J.Wenninger - LEP fest10 Underground Water  Underground water Rainfall  Lake levels  Other ? 1993 : Unexpected energy “drifts” over a few weeks were traced to cyclic circumference changes of ~ 2 mm/year. Circumference change measured with the radial beam position. Driving “forces” :

J.Wenninger - LEP fest11 The Crack in the Model Spring of 1994 : the beam energy model seemed to explain all observed sources of energy fluctuations... An unexplained energy increase of 5 MeV was observed in ONE experiment. It will remain unexplained for two years… EXCEPT :

J.Wenninger - LEP fest12 The Field Ghost  Short term fluctuations Long term increase (hysteresis) Energy increase of ~ 5 MeV over a LEP fill ! Quiet periods in the night ! The data showed (unexpected) : Human activity ! But which one ?? Summer 1995 : the first field measurements inside ring dipoles.

J.Wenninger - LEP fest13 Pipebusters The explanation was given by the Swiss electricity company EOS... Vagabond currents from trains and subways Vagabond currents from trains and subways Source of electrical noise and corrosion (first discussed in …1898 !) I blast your pipes ! ~20% ~80% Vagabond (Earth) current DC railway

J.Wenninger - LEP fest14 Vagabonding Currents  Injection lines (Point 1)  Point 6 (Versoix river) LEP is affected by the French DC railway line Geneva-Bellegarde A DC current of 1 A is flowing on the LEP vacuum chamber. Entrance/exit points :

J.Wenninger - LEP fest15 TGV for Paris  The current on the railway tracks  The current on the vacuum chamber  The dipole field in a magnet correlate perfectly ! Because energy calibrations were usually performed : At the end of fills (saturation)  During nights (no trains !) we “missed” the trains for many years ! we “missed” the trains for many years ! November 1995 : Measurements of

J.Wenninger - LEP fest16 Epilogue More than hour days of machine time were devoted to energy calibration between 1993 and The mass and width of the Z boson were measured with a remarkable accuracy (see forthcoming talks). The beam energy contributes ~ 1.5 MeV to the total errors. Work is in progress on for the W mass... The LEP Energy Calibration Working Group was a very successful collaboration between physicist from the machine and the experiments, building ties between the two communities. Many other effects besides tides and trains are included in the LEP energy model. There is not enough time to give details... 5 years ( ) were needed to unravel most of the beam energy “mysteries”.

J.Wenninger - LEP fest17 LEP Laser Polarimeter