the bessy low alpha optics and the generation of coherent synchrotron radiation
DESCRIPTION
The BESSY Low Alpha Optics and the Generation of Coherent Synchrotron Radiation. J. Feikes, K. Holldack, H.-W. Hübers*, P. Kuske, G. Wüstefeld BESSY and * DLR, BERLIN. ‘Frontiers of Short Bunches in Storage Rings’ Frascati, INFN, 7-8 November 2005. - PowerPoint PPT PresentationTRANSCRIPT
The BESSY Low Alpha Optics and the Generation of Coherent Synchrotron Radiation
J. Feikes, K. Holldack, H.-W. Hübers*, P. Kuske, G. WüstefeldBESSY and * DLR, BERLIN
see contribution in ICFA Beam Dynamics Newsletter No. 35, December 2004
‘Frontiers of Short Bunches in Storage Rings’ Frascati, INFN, 7-8 November 2005
Content
G. Wüstefeld et al., BESSY Low Alpha Optics, Frascati, 7-8 Nov. 2005
1. Low alpha optics 2. Coherent radiation3. Bunch-length current relation4. Limits of short bunches 5. Upgrade option: short bunches at BESSY II
content
the machine opticsoptics parameter reg.user
optics
low alpha
optics
circumference / m 240 240
number of cells 2x8 16
nom. Energy / GeV 1.7 1.7
tunes Qx / Qy 17.8 / 6.7 14.7 / 6.2
nat. chrom x / y -53 / -27 -35 / -27
nat. emitt / nmrad 6
synchr. freq. / kHz 7.5 7.5 … 0.35
mom. com. factor 7.2E-4 7E-4 …1E-6
plus & minus
nat. bunch length rms / ps 12 12 … 0.7
main parameters
short bunches by low manipulation ²fs = control value
very stable machine operation, good life time 20 mA and 20 hours
application: coherent THz radiation, ICFA No. 35, article by U. Schade et al. short x-ray pulses at BESSY, accepted PRL, A. Krasyuk et al., 2005
G. Wüstefeld et al., BESSY Low Alpha Optics, Frascati, 7-8 Nov. 2005
The BESSY Low Alpha Optics
single & multi bunch1.25 MHz to 500 MHz10 A < I< 0.1 mA(2mA~10 electrons)
10
4 sextuple familiesfor beam dynamicscorrections
α=-3·10-6
fs=350Hz
synchrotron frequency and alpha
synchrotron frequency fs as a function of rf frequency
- fs increases strongly with deviating rf frequency - optics tuned by sextupoles (long. chromaticity)
extracted momentum compaction factor
- fit to measured data
2210
03.0,0,103 216
0 rms
G. Wüstefeld et al., BESSY Low Alpha Optics, Frascati, 7-8 Nov. 2005
Longitudinal tune
=0.1%
temporal resolved THz pulse of pulse length of few 100 ps:multiple reflections in THz beam line
H.-W. Hübers et al.Applied Phys. Lett.87,184103 (2005)
InSb-bolometer
resolution of single turns, =1s
1 turn
1 turn
bursting CSR
stable CSR
CS
R in
tens
ityC
SR
inte
nsity
time
G. Wüstefeld et al., BESSY Low Alpha Optics, Frascati, 7-8 Nov. 2005
THz Detectors at BESSY
Typical values Si-Bol. InSb HEB
NEP (W/Hz1/2) ~10-13 ~10-12 ~10-10
Rise time (ns) ~106 ~1000 ~0.03
Frequency (THz) 0.1 - 15 0.1 -1.5 0.3 - 6
Detector parameters
H.-W. Hübers et al.,ICFA Newsletter No. 35
hot-electron bolometer HEB
resolution of single bunches, =30ps
Spectral range of CSR
G. Wüstefeld et al., BESSY Low Alpha Optics, Frascati, 7-8 Nov. 2005
power spectrum analysis by Martin-Puplett Fourier transform spectrometer
Brilliance of the BESSY THz spectrum
10 gain710 gain
7
1 10 100 1000 1000010-14
10-9
10-4
101
low alpha stable CSR, 18 mA
user optics burstig CSR, SB 15 mA
0.1THz 1THz
black body, 1200 K, 10 mm^2
incoherent radiation250 mA, user optics
BR
ILLI
AN
CE
[W
/mm2 /s
r/(0
.1%
bdw
)]
WAVENUMBER [cm-1]
raw data power spectruminterferogram source comparison
user optics, single bunch 15 mA
Power spectrum and bunch shape of stable bunches
G. Wüstefeld et al., BESSY Low Alpha Optics, Frascati, 7-8 Nov. 2005
CSR bunch length measurement
- 700 fs, 300 nA- 870 fs, 140 nA- 1.2 ps, 140 nA
- fit
Fourier transform spectroscopy,coherent and incoherent THz radiation interferogram
Fourier transform of interferogram power spectrum, raw data includes f()-factor
experimental dataTHz pulses
Theorymachine parameters
Haïssinski equation and CSR wake bunch shape n(z)
Fourier transform of bunch shape form factor g()
Kramers-Kronig analysis shape of THz pulse 122 /1 z
Gaussian relation between bunch length and spectral band width
normalized power spectrum
power spectrum coherent • f()power spectrum incohere.• f() = P / Pcoh. incoh.
incohere. power P = p Ncoherent power P = p N (N -1)g() norm. power spectrum P / P = N g()coh
incoh
coh
incohee
e
e
no significant difference was found in thespectral distribution for <0 and >0
CSR spectra at fs=1.75 kHz, =3 psdifferent 400-bunch currents
raw data, not normalized
wavenumber 1/cm
0
5
109.03mA8.10mA6.70mA4.50mA3.20mA2.20mA
0 10 20 30 400
10
9.96mA8.12 mA7.00mA5.00mA1.00mA
inte
nsity
/ a.
u.in
tens
ity /
a.u.
< 0
> 0
G. Wüstefeld et al., BESSY Low Alpha Optics, Frascati, 7-8 Nov. 2005
Example of THz power spectra taken at IRIS (BESSY)
higher currents expand the spectrum to higher frequencies:
-stable bunch deformation-unstable bunch bursting
normalized
by I²
Pcoh/Pincoh
CSR spectra at fs=1.2 kHz and different currents
Fourier transform measurements at the BESSY IRIS infrared beam line,cooperation with Dr. Ulrich Schade (BESSY), Dr. Jongseok Lee (Seoul National University)
THz optics3 ps
user optics13 ps
sub-ps optics700 fs
bursting instabilityStupakov & Heifets
streak camera data
THz databursting data
2/30
40
40 )/()/()/( IIff
scaling relation between bunch length synchrotron frequency f and current I:
sin
gle
bu
nch
cu
rren
t /
mA
bursting frequency / kHz
temporal emission spectrum of CSR bursts (user optics)
bunch length - current relation
G. Wüstefeld et al., BESSY Low Alpha Optics, Frascati, 7-8 Nov. 2005
Bunch length and current relation
bursting data
~I 0.384
~I 3/7
~I 3/8
single bunch current / mA
bunc
h le
ngth
/ p
s
results from bursting threshold:
- eff. / naturale bunch length = 1.5
- eff. bunch length · unstable mode k =5
- bunch length ~ current relation ~I ª
a=3/8 from experiments, a=3/7 from theory
0
ii
linear coupling matrix, long.-horiz. ,the chromatic H-function couples the planes:
)'(' 1561551521512 zmzmxmxmz
126121622126111621152151 )()( xmmmmxmmmmxmxmz
1000
1
0
0
565251
262221
161211
mmm
mmm
mmm
Mx-z transfer matrix, no energy change
use transformation properties of dispersive vector (D,D’) to replace m16 and m26
12 xMx
x’ D’
x1/2
DH1/2
Hxx
222111 sinsin HxHx HHz
G. Wüstefeld et al., BESSY Low Alpha Optics, Frascati, 7-8 Nov. 2005
Limits of short bunches I
similar expression for m55 & m56 - terms, if z’ and are included!
0.45 MV45.0 MV
rf-voltage:
scheme of presently constructed MLS ring of the PTB, next to BESSY site
Emax=600 MeVcircumference = 48 m
longitudinale bunch length is chromatic H dependent
x-x’ x-x’z-z’z-z’
port IIH=1.2 rad·m
port IH=0.035 rad·m
bunch length / mmbunch length / mm
G. Wüstefeld et al., BESSY Low Alpha Optics, Frascati, 7-8 Nov. 2005
Limits of short bunches II
quadrupoles ~ sextupoles ~ d/doctupolesd /d
22
low alpha tuning:
=1.0 mm =0.1 mm
=1.0 mm =0.5 mm
t
MAD tracking simulation,8·10 turns = 10damping times & quantum excitation
5
BESSY II, user optics: MAD-simulation of electron diffusion due to radiation damping
¯
¯longitudinal delay / ps
rela
tive
mo
me
ntu
m d
ev
iati
on
‰
bunch rotation90 degree
¯longitudinal delay / ps
nu
mb
er
of
ele
ctr
on
s
/ a
.u.
bunch rotation 180° quantum excitation
¯
2
3
4
5
6
7
8
9
1
0 1.6 3.3 5.0-5 -3.3 -1.6
-rms=0.4 mm
conclusion: radiation damping limits the multiple usage of - ‘laser sliced’ electrons for short x-rays - ‘laser sliced’ dip as a THz-source
G. Wüstefeld et al., BESSY Low Alpha Optics, Frascati, 7-8 Nov. 2005
Limits of short bunches III
180° in phase long. space
80 turns around machine
initial value: no spread in phase space, only natural spread in momentum distribution
long. bunch length spread of =0.4 mm
Upgrading of the rf-gradient
G. Wüstefeld et al., BESSY Low Alpha Optics, Frascati, 7-8 Nov. 2005
option for enhanced THz radiation and short X-ray pulses at BESSY II:
upgrading the rf-gradient by a 1.5 GHz, cw superconducting rf-structure placed into one straight ID-section
applied scaling law for bursting threshold: dzdVI rfz /3/8
figure copied from F. Sannibale et al, ICFA Newsletter No. 35
BESSY II 710 Auser optics & upgrade
upgrading by a factor of 201000 x more THz power!
upgrading by a factor of 100sub-ps bunches!
single bunch current / mA
rms-
bunc
h le
ngth
/ ps
user optics
user optics
THz optics
THz optics
0.5 GHz &
1.5 MV
1.5 GHz &
50 MV
bursting threshold
bursting threshold
present rf
upgraded rf
13 ps
3 ps
1.3 ps
0.3 fs
Conclusion
G. Wüstefeld et al., BESSY Low Alpha Optics, Frascati, 7-8 Nov. 2005
Conclusion:
the low alpha optics (as one possible scheme) extends the usage of storage rings to intense THz and short X-ray pulses
coherent THz radiation as a diagnostics tool delivers sensitiveand new information on beam dynamics