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J.B. Rosenzweig and Scott Anderson

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Title: J.B. Rosenzweig and Scott Anderson


1
The Role of Space-charge in Emittance Measurement
of High-brightness Photoinjector Beams
  • J.B. Rosenzweig and Scott Anderson
  • UCLA Dept. of Physics and Astronomy
  • ICFA Sardegna, July 2002

2
Measuring the emittance of photoinjector beams
  • The low emittance of, and huge forces (internal
    and external) applied to these beams makes them
    behave very differently (like plasmas) than
    emittance dominated beams
  • In addition, investigation of the behavior of
    these beams, as well as optimization of the
    beams end use, requires accurate measurement of
    the beam emittance
  • In order to produce accurate measurements, the
    emittance diagnostic must take into account the
    nature of photoinjector beams

3
Measuring Emittance
  • Traditional emittance measurement techniques
    (e.g. quadrupole scan) use the envelope equation
    for a drifting beam ignoring space-charge,
  • For typical photo-injector beams, this exclusion
    of the space-charge term is not appropriate
    except in a strongly focused waist. We see that
    these beams are space-charge dominated by the
    ratio of the space-charge to emittance terms in
    the full envelope equation.
  • We used the LLNL/UCLA Thomson scattering
    photoinjector, with a short pulse, low energy
    beam to test different emittance measurement
    techniques.

4
Slit Based Emittance Measurement
  • Beam phase space is reconstructed from the
    position and width of the beamlets on screen.
    Emittance calculated from phase space picture.
  • Collimation makess emittance dominated beamlet
    expansion due to emittance, not space-charge.
    Plasma wavelength same b function becomes much
    smaller.

5
Quadrupole Scan Measurements
  • Neglecting space charge we can write an equation
    for s2 based on the Twiss parameters of the beam.
  • The procedure then, is to measure s2 (the mean
    square beam size) versus the focal length of the
    lens and fit the resulting curve to calculate the
    emittance.
  • Thick lens treatment often necessary in compact
    beamlines.

6
Experimental Procedure
  • Emittance was measured using both the quad scan
    and slits for different beam plasma frequencies.
  • The plasma frequency was changed by changing the
    laser pulse length. This was done by altering
    the grating pair separation in the laser system.
  • For each set of measurements, the laser spot size
    and energy, grating pair separation, beam charge,
    and injection phase were recorded in order to
    calculate the plasma frequencies.

7
Quad Scan Vs Slit Data
The strength of the space-charge forces are
parameterized in the scan by product drift length
between quadrupole and detector and the plasma
wave number.
8
Simulation of the Quad Scan
  • Given the measurements of charge and laser pulse
    dimensions, we simulated the beam dynamics up to
    the quadrupole using PARMELA and HOMDYN.
  • The quad scan procedure was then simulated with
    PARMELA using point to point space charge,
    HOMDYN, and by integrating the envelope equation.
  • All three methods gave similar results. Linear
    transport models agreeing with PARMELA leads us
    to believe non-linear space charge effects are
    unimportant.

9
Quad Scan Simulation
  • PARMELA simulations predict emittances in good
    agreement with slit measurements.
  • Simulated quad scans with emittances set by the
    slit measurements give higher output emittance
    values that agree reasonably with quad scan
    measurements.

10
Space-charge in the Quad Scan
  • There are two relevant normalized numbers two
    parameterize space charge strength, one measuring
    drift length, and the other measuring emittance
    v. space charge.
  • The white plot points locate the positions of the
    experimental data. The normalized emittance used
    as input to the simulations was 5 mm mrad.
  • kpb is a measure of the ratio of the space-charge
    to emittance forces at the quadrupole.

11
Interplay of Space-charge and Emittance
Simulation
  • Data and simulation both show asymmetry about
    minimum spot size.
  • Asymmetry is due to different emittance forces.
    If waist is emittance dominated, then envelope
    looks very different before and after waist.
  • Asymmetry makes fitting to a parabola
    problematic.

12
Summary of Emittance Measurement Techniques
  • Quad scans are ill-suited for highly space-charge
    dominated beams because the beam evolves under
    the influence of both space-charge and emittance
    effects.
  • Rules of thumb
  • Quad scan data may not be valid if
  • Asymmetry in the data is an indicator of trouble.
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