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Lowering SEY by Rough Surfaces I. Montero L. Aguilera, L. Galán, V. Nistor, J.L. Sacedón, M.Vázquez F. Caspers, D. Raboso. Anti e-cloud coatings, AEC’09 CERN. AEC’09 I. Montero CERN 12.10.09. Main goal: - PowerPoint PPT Presentation
Citation preview
Lowering SEY by Rough Surfaces
I. Montero
L. Aguilera, L. Galán, V. Nistor, J.L. Sacedón, M.Vázquez F. Caspers, D. Raboso
Anti e-cloud coatings, AEC’09 CERN
Main goal:
Avoid multipactor discharge by low secondary
electron emission coatings
Support:
AEC’09 I. Montero CERN 12.10.09
AEC’09 I. Montero CERN 12.10.09
Outline
Anti-Multipactor Coatings for SpaceLow secondary electron emission coatings
Stability with exposure to air (months)
Secondary Electron Emission Suppression Surface Roughness of High Aspect Ratio:
Chemical Etching methodsMicro-Particulated surfaces
Nano-structured surfacesMagnetic Materials
Summary and Conclusions
AEC’09 I. Montero CERN 12.10.09
Outline
Anti-Multipactor Coatings for SpaceLow secondary electron emission coatings
Stability with exposure to air (months)
Secondary Electron Emission Suppression Surface Roughness of High Aspect Ratio:
Chemical Etching methodsMicro-Particulated surfaces
Nano-structured surfacesMagnetic Materials
Summary and Conclusions
• Low secondary electron emission • High first cross-over energy• Low surface RF resistance• Stability with exposure to air (months)
Conditioning in situ, not possible heat treatments electron beams ion beams
Anti-Multipactor Coatings for
Space
EXPOSURE TO AIRMETAL
LOW SEY LOW Rsurf
OXIDE
HIGH SEY HIGH Rsurf
Time / Reactivity
REQUIREMENTS
Conditioning
AEC’09 I. Montero CERN 12.10.09
Deposition techniques:
Cr and Ti silicides:coevaporation with ion assistance
hydrogenated and nitrogenated
amorphous carbon: reactive evaporation with ion
assistance, plasma
Ti, V, and Cr nitrides and carbides, reactive evaporation or sputtering
with ion assistance
0.5
1.0
1.5
2.0
SE
Y
clean
air-exposed
Au
Alo
din
e
Nb
N
TiC
TiN
VN
CrN
a-C
:H
a-C
N:H
CN
TiS
i
CrS
i
COATINGS
Initial Selection of Potential Materials
AEC’09 I. Montero CERN 12.10.09 Stability with exposure to air
(months)Previo
us
results
Effect of exposure to air on SEY
(months)
SEY OF VN SEY OF CrNSEY OF TiN
0
5
10
15
20
25
1E-12 1E-10 1E-08 1E-06 0.0001 0.01 1 100
Time of Exposure to Air [day]
SEE
FoM
[eV
1/2
]
TiN/Ti ion implantation
TiN/Ag evaporation
TiN/Al evaporation
TiN/Au evaporation
TiN/Al evaporation
TiN/Si sputtering
TiN/Ag cathodic arc
TiN/Rh/Ag evaporation
Alodine 1200 (ESTEC)
c)
AEC’09 I. Montero CERN 12.10.09
SEY FoM (E1/m)1/2 E1 = Firt cross-over energym= SEY maximum
AEC’09 I. Montero CERN 12.10.09
Outline
Anti-Multipactor Coatings for SpaceLow secondary electron emission coatings
Stability with exposure to air (months)
Secondary Electron Emission SuppressionSurface Roughness of High Aspect Ratio:
Chemical Etching methodsMicro-Particulated surfaces
Nano-structured surfacesMagnetic Materials
Summary and Conclusions
Silver 40 μm
Electroplating Ni + Ag
SilverSilver Silver
Nickel 10 μm
Micro-structured Gold
Coating
Chemical Etching and Sputtering
Methods
Nickel 10 μm Nickel 10 μm
Chemical etching
Aluminum alloy device
Aluminum alloy device
Aluminum alloy device
silver Gold
AEC’09 I. Montero CERN 12.10.09
Sputtering method
Micro-structured Gold
Coating
Chemical Etching and Sputtering Methods
Anti-Multipactor Coatings for Space
it is possible by secondary emission suppression by surface roughness of high aspect ratio
AEC’09 I. Montero CERN 12.10.09
0.0
0.5
1.0
1.5
2.0
2.5
0 200 400 600 800 1000 1200 1400Primary Electron Energy [eV]
SE
E c
oefic
ient
Ag plated
chem. etched
Au coated
Au / c-Si
WR75 12 GHz transformer 0.14 mm gap
E1
AEC’09 I. Montero CERN 12.10.09
Outline
Anti-Multipactor Coatings for SpaceLow secondary electron emission coatings
Stability with exposure to air (months)
Secondary Electron Emission Suppression Surface Roughness of High Aspect Ratio:
Chemical Etching methodsMicro-Particulated surface
Nano-structured surfacesMagnetic Materials.
Summary and Conclusions
Angular dependence of secondary emission yield
EmpiricalVaughanIEEE (1989)IEEE (1993)
Empirical ( MEST)
AEC’09 I. Montero CERN 12.10.09
= electron incident energy= angle of incidence measured with respect to the surface normal, max SEY max.at normal incidence.ksd and ksw = rough surface parameters (both can vary between 0 for rough surfaces and 2 for polished)
Aluminum alloy substrate
Sprinkled Al particles
Al particles / SEY ((Incidence Angle)
0.0
0.5
1.0
1.5
2.0
2.5
3.0
0 200 400 600 800 1000Primery Electron Energy (eV)
SE
Y
Al particl -5º
Al particl 0º
Al particl 10º
Al particl. 25º
Al particl. 35º
Al particl. -20º
Al particl. -35º
Al particl. -45º
Aluminium foil /SEY (Incidence Angle)
0.0
0.5
1.0
1.5
2.0
2.5
3.0
0 200 400 600 800 1000Primary Electron Energy (eV)
SE
Y
Al foil-5º
Al foil 0º
Al foil 10º
Al foil 25º
Al foil 35
Al foil -20º
Al foil -35º
Al foil -45º
Flat surface
Angular dependence of secondary emission yield
Aluminum alloy substrate
AEC’09 I. Montero CERN 12.10.09 Conductive particulated
surfaces
Gold-Coated Aluminum Particles
Sputtering 5 nm AuSprinkled Al particles
Aluminum alloy substrate
Au / Al particles
0,0
0,2
0,4
0,6
0,8
1,0
1,2
1,4
1,6
0 200 400 600 800 1000
Primary Electron Energy (eV)
SE
Y
Al part +Au-312ºAl part +Au-317ºAl part +Au-327ºAl part +Au-342ºAl part +Au-352ºAl part +Au-297ºAl part +Au-282ºAl part +Au-272º
AEC’09 I. Montero CERN 12.10.09
0.00000
0.00005
0.00010
0.00015
0.00020
0.00025
200 500 SEYMax
Primary Electron Energy (eV)
Roughnes
s fa
ctor
Al partículas
Al part+Au
Al foil
AEC’09 I. Montero CERN 12.10.09 Angular dependence of secondary emission yield
SEY a2-b+cSimple aproximation
a
The effect of angle is more sensitive a lower
energies
Aluminum
0.8
1.0
1.2
1.4
1.6
1.8
2.0
2.2
270 290 310 330 350
Incidence Angle
SE
Y
Al part- SEYMax
Al part+Au- SEYMax
Ep = Emax
Aluminum foil
y = 0.00018183x2 - 0.11367224x + 20.17658972R2 = 0.96478276
2
2.1
2.2
2.3
2.4
2.5
2.6
2.7
2.8
260 280 300 320 340 360
incidence angle (sample manipulator)
SEY
(normal incidence 313º)
Ep = Emax
5030 5010-10-30-50
AlFlat surface
3010-10-30-50
Micrometrical Dielectric Particles
CoatingFrom suspension of nano-metrical Al2O3 particles
Aluminum alloy substrate
Al2O3
Indentation of micro-metrical ceramic particles
Aluminum alloy substrate
0.0
0.5
1.0
1.5
2.0
2.5
0 400 800 1200 1600 2000Primary Electron Energy [eV]
SEE
coef
ficie
nt
25 nm Au coating (continuous)
as prepared (pulse)
25 nm Au coating (pulse)
AEC’09 I. Montero CERN 12.10.09
0.0
0.5
1.0
1.5
2.0
2.5
3.0
0 200 400 600 800 1000Primary Electron Energy [eV]
SE
E c
oeff
icie
nt
continuous technique
pulse technique
SEY
0,0
0,2
0,4
0,6
0,8
1,0
1,2
1,4
1,6
1,8
2,0
0 200 400 600 800 1000Primary Electron Energy (eV)
SE
Y c
oe
ffic
ien
t
Al2O3 75%+Al 25%+Au
Al2O3 50%+ Al 50% +Au
Al2O3 25%+ Al 25% +Au
Metallic/Dielectric Microparticles
Coatings
Al particle
Al2O3 particle
Surface top view
AEC’09 I. Montero CERN 12.10.09
Extreme reduction of SEY
Gold coated
SEY
0,0
0,5
1,0
1,5
2,0
0 500 1000 1500 2000 2500 3000 3500 4000
Primary Electron Energy (eV)
SE
Y c
oef
fici
ent
Al2O3 75%+Al 25%+Au
Al2O3 50%+ Al 50% +Au
Al2O3 25%+ Al 25% +Au
Metallic/Dielectric MicroParticle
Mixture Al particle
Al2O3 particle
Surface top view
AEC’09 I. Montero CERN 12.10.09
Gold coated
AEC’09 I. Montero CERN 12.10.09
Outline
Anti-Multipactor Coatings for SpaceLow secondary electron emission coatings
Stability with exposure to air (months)
Secondary Electron Emission Suppression Surface Roughness of High Aspect Ratio:
Chemical Etching methodsMicro-Particulated surfaces
Nano-structured surfacesMagnetic Materials
Summary and Conclusions
Outer oxide
Nanostrured anodic aluminium oxide
templates
AEC’09 I. Montero CERN 12.10.09
100 nm
SEM Image of the Aluminium
Anodic Oxide
Porous-type Alumina Barrier-type Alumina
Aluminium
Inner-oxide
Gold coated
2,8
2,8
2,8
2,9
2,9
2,9
2,9
2,9
3,0
270 290 310 330 350
Incidence Angle
SEY
Anod24h
0,0
0,5
1,0
1,5
2,0
2,5
3,0
3,5
0 200 400 600 800 1000Primary Electron Energy (eV)
SE
Y
Anodización 24h-312º
Anodización 24h-342º
Anodización 24h-282º
Anodización 24h-317º
Anodización 24h-307º
Anodización 24h-327º
Anodización 24h-297º
AEC’09 I. Montero CERN 12.10.09 Nanostrured anodic aluminium
oxides
Image of the AluminiumçAnodic Oxide Sample
0,0
0,2
0,4
0,6
0,8
1,0
1,2
1,4
1,6
1,8
2,0
0 200 400 600 800 1000Primary Electron Energy (eV)
SE
Y c
oeffi
cien
t
Anodización 24h+Au-312º
Anodización 24h+Au-317º
Anodización 24h+Au-307º
Anodización 24h+Au-327º
Anodización 24h+Au-297º
Anodización 24h+Au-342º
Anodización 24h+Au-352º
1,6
1,7
1,7
1,8
1,8
1,9
1,9
2,0
2,0
270 290 310 330 350Incidence Angle
SE
Y SEYMax
AEC’09 I. Montero CERN 12.10.09 Gold coated Nanostrured anodic aluminium
oxides
() = cte.
Outline
Anti-Multipactor Coatings for SpaceLow secondary electron emission coatings
Stability with exposure to air (months)
Secondary Electron Emission Suppression Surface Roughness of High Aspect Ratio:
Chemical Etching methodsMicro-Particles
Nano-structured surfacesMagnetic Materials
Summary and Conclusions
AEC’09 I. Montero CERN 12.10.09
Magnetic suppression of
SEY
AEC’09 I. Montero CERN 12.10.09
target
Magnetic field
SEY suppression will be achieved through the reduction of the local electric field near the surface of the sample by this virtual cathode,
and further secondary electrons emitted in this low electric field environment could be reabsorbed.
D. J. Rej, et al. J. Vac. Sci.Technol. B 12, 861 1994
a magnetic field II to the sample surface would confine a layer of secondary electrons near the surface, forming a virtual cathode.
Virtual CathodeEmitted electrons
Ing Hwie Tan, J. Appl. Phys. 100, 033303 2006
e-e-
Ferrite FeTi
0.0
0.5
1.0
1.5
2.0
2.5
3.0
3.5
4.0
0 100 200 300 400 500 600 700 800 900Primary Electron Energy (eV)
SE
Y C
oeffic
ient
AEC’09 I. Montero CERN 12.10.09
NiZnC and MnZn powders
SEY
0.00
0.20
0.40
0.60
0.80
1.00
1.20
1.40
1.60
0 500 1000 1500 2000 2500 3000 3500 4000
Primary Electron Energy (eV)
SE
Y c
oef
fici
ent
MnZn/Cu
NiZn/Cu +Au
SEM
Magnetic Materials
SEY max>1with and without gold
AEC’09 I. Montero CERN 12.10.09
0.0
0.2
0.4
0.6
0.8
1.0
1.2
1.4
1.6
1.8
2.0
0 1000 2000 3000 4000Primary Electron Energy (eV)
SE
Y c
oeffic
ient
magnetic viewer cards
Magnetic sample
magnetic domains
Magnetic Materials
Aluminum alloy substrate
Gold coated Micrometrical Magnetic
Particles MagneticMicro- particles
AEC’09 I. Montero CERN 12.10.09
0.0E+00
1.0E-05
2.0E-05
3.0E-05
4.0E-05
5.0E-05
6.0E-05
7.0E-05
8.0E-05
9.0E-05
200 500 Sey max
Primary electron energy (eV
Roughnes
s fa
ctor
Ferrita part+Au
Ferrita part+Au+Hilos H
Ferrita part+Au+Hilos V
0.0
0.2
0.4
0.6
0.8
1.0
1.2
0 200 400 600 800 1000Primary Electron Energy (eV)
SE
Y c
oeff
icie
nt
Ferrita+Au-312º
Ferrita+Au-342º
Ferrita +Au-300º
Ferrita +Au-352º
Ferrita +Au-352º
ferrite
gold
Magnetic Materials
Summary and Conclusions
Rough low-SEY surfaces can “suppress” significantly secondary emission yield
Rough coatings shows high 1st-crossover-
energy
Multipactor effect can be suppressed using
rough surfaces of adequate morphology
The “suppression” of SEY of rough coatings is
more effective at low primary energies, where
it affects more to multipactor
Surface roughness should be in the micro scale.
AEC’09 I. Montero CERN 12.10.09
Cont.
Low electrical resistivity is now more important since roughness increases surface resistance
Strong roughness for SEY suppression could implies highly porous coating with poor
mechanical properties. Silver and gold required for their electrical conductivity are too soft.
Gold is more stable in air but has bad adherence.
ECM'08 (Electron Cloud Mitigation 2008)
AEC’09 I. Montero CERN 12.10.09
Cont.
Rough surfaces has the ability to absorb
partially emitted electrons for any incident
direction of primary electrons.
We have made several efforts to achieve near-total supression of SEY using particulated
surfaces. Here we have showed that near total
absorption of electrons can be achieved in metal/dielectric particulated coatings. The
effect is realized over a wide range of incident primary energy .
AEC’09 I. Montero CERN 12.10.09
Cont.
The SEY curves do not seem to be explained by known simulations for rough surfaces
Magnetized surfaces, apart from surface roughness, will be investigated to explain these
results.
They deserve further research on their potential application
AEC’09 I. Montero CERN 12.10.09
Thank you for your attention
SEE Yield Measurements on InsulatorsCharging on insulators alters
electron yields.
SE’s
Vbias = 0 Vbias < 0 Vbias > 0
Experimental Technique:• Pulsed beam current <100nA, <700ns
Q < 106 electrons/pulse
10-100 mV/pulse• Neutralization methods
Flood gun, and VUV neutralization for repeated electron pulsed yields at 200 eV
• low noise level
ECM'08 (Electron Cloud Mitigation 2008)