Injection and extraction, single turn injectionplumma/Plum_3_single_turn_inj.pdfof circulating and...
Transcript of Injection and extraction, single turn injectionplumma/Plum_3_single_turn_inj.pdfof circulating and...
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USPAS
Injection and extraction, single turn injection
USPAS
by Mike Plum and Uli Wienands
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USPASIntroduction
• What do we mean by injection?Inject a particle beam into a circular accelerator or accumulator ring, at the right time, whileminimizing the beam loss and placing the newly injected particles onto the correct trajectorywith the correct phase-space parameters
• What do we mean by extraction?Extract the particles at the appropriate time, whileminimizing beam loss andplacing the extracted particles onto the correct trajectorywith the correct phase-space parameters
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USPASIntroduction (cont.)
• Why do we care about injection and extraction?If it is not done right, the accelerator facility won’t work rightInjection and extraction can be the most complex parts of a ring (e.g. the injection area of the SNS has the most complex optics in the accelerator facility)Once commissioning starts, issues concerning injection and extraction often come up due to unanticipated factors (e.g. PSR, SNS, …)A good understanding of injection and extraction will lead to better design, fabrication, installation, and operation of your accelerator facility
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USPASBasic difference between inj and extr.
• Beam energy at injection is often lower than at extractionSpace charge forces are higher because there is little cancellation of the magnetic and electric forces at low beam energyTransverse oscillation amplitudes are smaller at high beam energies due to adiabatic damping (see section on normalized emittance)
p
p
p
p
Two protons just sitting still will repel
Two protons traveling at the speed of light will neither repel or attract
Space charge cartoon
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USPASEmittance vs. beam energy
xεβ
xεγ
x’
x
Beam Ellipse in Phase Space:∫ = πεdxdx'The ellipse area,
is not invariant when the particles are accelerated. But if we substitute transverse momentum, px, in place of x’, it will be invariant
εn is the normalized emittance, and it is invariant when the beam is accelerated
βγεε =n
These β and γ are the relativistic parameters!
*
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USPASEmittance vs. beam energy (cont.)
Beam sizeβγβε
εβσ xnxx ==
The normalized emittance is constant, so as the beam is accelerated, the beam size gets smaller (for a given Twiss parameter βx )
This is known as adiabatic damping
βγεε =n
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USPASInjection system components• Beam line transport up to the ring• Beam transport to a dump for particles that are not
properly injected• RF cavities to paint beam longitudinally• Septum magnet• Magnets that merge incoming and circulating beams• Bump magnets• Stripper foils (charge exchange injection)• Kicker magnet (single turn injection)
Example: SNS Ring injection area
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USPASMagnetic septum
Soft iron Laminated yoke
Return coilSeptum coil
B0B=0
I
Bo = μ0I / g
Typically Ι 5-25 kA
(Courtesy B. Goddard)
(Courtesy BNL)
Example: SNS injection septum magnet
Example: SNS injection dump gradient septum magnet
(Courtesy BNL)
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USPASElectrostatic septum
E0 E=0
High voltageelectrode Hollow earth
electrode
Thin wire orfoil (~0.1 mm)
High VoltageElectrode
Hollow earthelectrodeSeptum wires
E = V / g
Typically V = 200 kV
E = 100 kV/cm
g
DC electrostatic device with very thin (~0.1mm)septum between zero field and high field region
(Courtesy B. Goddard)
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USPASInjection bump magnets
Example: SNS injection bump magnets. Max rate of change is 1400 Amps in 250 usec. Ceramic vacuum chamber first coated with copper, then TiN.
• Bump magnets, also known as kicker magnets, have magnetic fields that can be quickly changed to paint the beam into the ring acceptance
• This means that magnets must have low inductance (τ = L/R)
• Also need pulsed power supplies• Must be aware of eddy currents in
metal vacuum chambers, which can distort the magnetic field and heat the vacuum chamber
• Ceramic beam pipes are often used, but then need to account for image currents
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USPASInjection chicane magnets
• Injection chicane magnets merge the injected and circulating beams.
• Sometimes use “C” magnets, with one open side, to fit “Y” shaped vacuum chambers
Example: SNS chicane magnet with the stripper foil changing mechanism
H- beam from Linac Thin
Stripping Foil
To InjectionDump
ThickSecondary Foil
pH0
H-Dipole magnets
H- beam from Linac Thin
Stripping Foil
To InjectionDump
ThickSecondary Foil
pH0
H-Dipole magnets
Example: SNS injection chicane
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USPASStripper foils
SNS diamond foilClose up showing SNS diamond foil corrugation
New style PSR foil
Old style PSR foil completely supported by carbon fibers
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USPASSingle turn injection
(Figure is from Bryant & Johnson, The Principles of Circular Accelerators and Storage Rings)
x
s
A maximum of one beam bunch is injected into each RF bucket
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USPASHill’s equations
0)(''
0)(''
=+
=+
ysKy
xsKx
y
x
rigidity magnetic/
/
)/()/(
//
2
==
∂∂≡′
′−≡+′≡
≡′≡′
−
qmvB
xBB
BBKBBKdsdyydsdxx
y
y
x
ρ
ρρρ
( )
( ) ( )[ ]
2/)()(
)(sin)(cos)()(
)(
)(cos)()(
ss
ssssAsx
ssAsx
βα
φψφψαβ
φψβ
′−≡
+++−=′
+=
• Equations of motion
where
• Solution:
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USPASBeam position and angle at the septum
( )
( ) ( )[ ] kssssAsx
ssAsx
δφψφψαβ
φψβ
−=+++−=′
=+=
)(sin)(cos)()(
)(
0)(cos)()(
At the kicker, where β(s) = βk we desire x(s) = 0 and x’(s) = -δk.
We will find the position and angle at the septum, x(0)=xs and x’(0)=x’s
Let α(0) = αs, and let the phase advance from the septum to the kicker be ψ(s) = μ
kkA βδ=
μ + φ = π/2
[ ] [ ]μαβ
μμαββδ
μββδ
cotcossin
sin
+−=+−=′
=
ss
ss
s
kks
skks
xx
x
(Beware that s is either a distance or designates the septum here)*
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USPASPractical considerations
Figure is from Bryant & Johnson, The Principles of Circular Accelerators and Storage Rings
x
s
xs must be greater than: n • (rms width of injected beam)
+ m • (rms width of circulating beam)+ (thickness of septum plate)+ (beam size increase due to energy spread)+ (closed orbit distortions)+ (alignment errors)n and m are factors to account for beam tails, typically 4 to 10
*
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USPASPractical considerations - kicker
μββδ
sinsk
sk
x=
• To keep the cost of the kicker down we would like to reduce the kick angle δ as much as reasonably possible
• Would like μ to be close to π/2• Would like large values of βk. (Note: large values of βs would
lead to large beam size, which would require larger separation of circulating and injected beam)
• The rise and fall time of the kicker must be fast enough that the field is practically zero when other beam bunches pass by the kicker (or for the case of just one bunch in the ring, when the head of the injected beam comes back around to the injection point)
• Typical rise and fall times are 50 to 150 ns. Typical voltage and currents are 40 to 80 kV and 2000 to 5000 A
Kicker angle(Courtesy B. Goddard)
μββδ sinskksx =
From solution on previous slide,
therefore,
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USPASPractical considerations - septum
• Septum bend angle must be great enough that the incoming beam will clear the ring magnets upstream of the injection point
• The stray field of the septum must be small in the vicinity of the circulating beam
• Stray fields are of greater concerns at lower beam energies• Electrostatic septa are weaker than their magnetic cousins,
but the partition, or septum, can be made very thin • Magnetic septum magnets are robust.• Typical fields are up to about 1 to 1.5 T.
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USPASPractical considerations - other
• It is desirable that the Twiss parameters of the injected beam equal the Twiss parameters of the ring at the point of injection. Otherwise the effective emittance of the circulating beam will grow.
This is not necessarily the case for multi-turn injection
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USPASSingle-turn injection – normalised phase space
X
Large deflection by septum
θ septum'X
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USPASSingle-turn injection
phase advance to kicker location
X
'X
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USPASSingle-turn injection
Kicker deflection places beam on central orbit
kick angle δk
X
'X
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USPASInjection errors
• Any residual transverse oscillation will lead to an emittance blow-up through filamentation
Error in septum angleError in ring kicker angleSteering error
• Beam position monitors can be used to find the source of the error (see next slide)
• A “transverse damper” system can be used to damp these oscillations
• Possible that injection trajectory is well corrected, but there is still an emittance blow-up through optical mismatch
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USPASInjection errors
kicker
bpm1 bpm2
phase μ ∼π/2 ∼π/2∼π/2
septum
Angle errorsΔθs,k
Measured Displacements
δ1,2
δ1 = Δθs √(βsβ1) sin (μ1 – μs) + Δθk √(βkβ1) sin (μ1 – μk) ≈ Δθk √(βkβ1)
δ2 = Δθs √(βsβ2) sin (μ2 – μs) + Δθk √(βkβ2) sin (μ2 – μk) ≈ -Δθs √(βsβ2)
Δθs Δθk
δ1
δ2
*
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USPASInjection oscillations
For imperfect injection the beam oscillates around the central orbit. 1
kicker θ error
X
'X
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USPASInjection oscillations
For imperfect injection the beam oscillates around the central orbit. 2
X
'X
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USPASInjection oscillations
For imperfect injection the beam oscillates around the central orbit. 3
X
'X
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USPASInjection oscillations
For imperfect injection the beam oscillates around the central orbit. 4
X
'X
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USPASFilamentation
• Non-linear effects (e.g. magnetic field multipoles ) cause amplitude dependent effects in particle motion.
• Over many turns, a phase-space oscillation is transformed into an emittance increase.
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USPAS
X
'X
Filamentation
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USPAS
X
'X
Filamentation
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USPAS
X
'X
Filamentation
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USPAS
X
'X
Filamentation
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USPASFilamentation
X
'X
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USPAS
X
'X
Filamentation
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USPAS
X
'X
Filamentation
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USPAS
X
'X
Filamentation
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USPAS
X
'X
Filamentation
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USPAS
X
'X
Filamentation
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USPASOptical Mismatch at Injection
x
x’
Matched phase-space ellipse
Mismatched injected beam
Particles oscillate with conserved C-S invariant: a = γ x2 + 2α xx’ + β x’2
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USPASOptical Mismatch at Injection
Filamentation fills larger ellipse with same shape as matched ellipse
x
x’
Turn 0
Turn N
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USPASRecap
• Accelerator components involved in injection• Single turn injection
Position and angle of incoming beam as a function of phase advance and kicker angleRequired separation of incoming and circulating beamsOptimum phase advance
• Injection errorsInjection oscillationsFilamentationMismatched injection
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USPASAcknowledgements
• Thanks to Brennan Goddard. Many of these slides were copied from his CAS course.
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USPAS
• backup slides