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Pinhole Measurement Approach to K Measurements using Spontaneous Radiation November 14, 2005 J. Welch, R. Bionta, S. Reiche Basic Layout Fundamental ... – PowerPoint PPT presentation

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1
Pinhole Measurement Approach to K Measurements
using Spontaneous Radiation
  • November 14, 2005
  • J. Welch, R. Bionta, S. Reiche

2
Basic Layout
Basic Scheme
Slit width must be small to get clean signal. 2
mm shown.
Useg 1 is worst case
3
Fundamental Measurements
  • Relative energy deviation of 1st harmonic
    photons
  • Relative energy deviation of electron beam

4
Derived Quantities
  • Electron beam angles x, y
  • ?K / K the relative difference between a given
    segment K and that of a reference segment

5
Experimental Procedure to Measure K
  1. All segments out, flatten orbit to a few times
    BBA quality. Need orbit angles less than 10
    micro-radians to avoid scraping 1st harmonic SR
    on vacuum chamber.
  2. Insert one segment, adjust slit width for
    constant angular size, scan slit position to
    minimize apparent ? K/K , energy jitter
    correction on.
  3. Remove segment, repeat with different segment.
    The difference in K is calculated from the
    difference in measured ? K/K for the two segments.

6
Simulation Procedure
  1. Set nominal values for reference and test
    segments and detector (Ks, detector geometry,
    machine parameters)
  2. Add random energy and beam orbit jitter
  3. Calculate expected 1st harmonic photon energy
    averaged over detector geometry
  4. Add random photon statistics noise, machine
    energy, and beam angle.
  5. Calculate ?K/K based on the noisy values. This
    becomes the measured value of ? K/K.
  6. Repeat one shot at a time.

7
Flux Spectrum in Simulation
  • Shifted interference function at constant flux
  • Valid for 1st harmonic photons over /- 10
    micro-radian range

8
Spectrum Verification Reiche/Ott Calculation
  • Essentially same agreement result for off axis
    radiation and radiation produced by detuned
    segments

9
Spectrum Verification line outs
  • Reich/Ott photons from 8000-8500 eV, from -1 mm
    to 1 mm at 145 m from source. Y line out is very
    similar.

10
Geometry Effects
  • Effect of finite detector size and offset
  • u1(0) is the theoretical on-axis resonant photon
    energy.

11
?K/K Calculation
  • ?K/K beam energy term photon energy term
    geometry term

Minimize
Measure
12
Aligning the Pinhole
Scan range / - 1 mm X and Y
Actual beam Axis 0.5, 0.5
  • Simple 2D scan, one shot per data point, 0.1 mm
    steps, no multi-shot averaging
  • Error is added to geometry term.

Measured Beam axis 0.33, 0.34
13
Photon statistics
  • Variance of mean photon energy due to photon
    statistics
  • Need 104 counts for 10-4 relative error in mean.
  • At minimum charge, there are at least 2 x 106
    photons incident on 0.1 x 1 mm detector.
  • Error is added to ?ltugt/ltugt term.

14
Simulated K Measurement
15
Simulation values used
  • Detector Model
  • Efficiency 1
  • Energy Sensitivity 1 eV / 8.275 keV
  • Size 0.1mm x 1.0 mm
  • Beam Model
  • Orbit jitter 25 sigma, position and angle
  • Energy jitter, 0.1 energy uncertainty 3x10-5.
  • Beam size, 36 micron sigma, beta 30 m.
  • Minimum charge, 0.2 nC.
  • Segment Model
  • Design values for K and positions, 113 periods

16
Detector Requirements
  • ?ltugt/ltugt sensitivity 1 x 10-4
  • Energy window 8000 - 8500 eV enough to include
    the 1st harmonic bandwidth and beam energy jitter
    effect.
  • Precisely movable slits with adjustable width.
  • Scan range of a few mm, x,y. Slit width range 0
    to a few mm.
  • Efficiency (counts per photon) 1 or better.

17
Global Alignment Tool?
  • ?? can be measured to better than 1 micro-radian
    with pinhole scan, globally!
  • x, y can then be integrated from slope, similar
    to method of autocollimator measurement for
    straightness.
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