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Fundamentals and Applications of
Plasma Filaments
L. Wöste
Fachbereich Physik der Freien Universität
[email protected]@physik.fu-berlin.de
Coworkers Cooperation partnersK. Stelmaszczyk J.-P. WolfP. Rohwetter J. Kasparian
W. Nakaema, M. Rodriguez, M. Rodriguez, H. H. WilleWille, , R. R. BourayouBourayou,, H. Zuoquiang, T. Fujii,R. Sauerbrey, A. Mysyrowicz, W. W. KalknerKalkner, , GG.. MéchainMéchain, Y. Petit, S. Henin, , Y. Petit, S. Henin, J. Yu, E. Salmon, G. Méjean, Y.Y.--B. André,B. André, L. Klingbeil, K. L. Klingbeil, K. RethmeierRethmeier
TheTeramobile Project was financed by CNRS, DFG and SNF
Fundamentals and Applications of
Plasma Filaments
Contents
− Formation of white light filaments− Formation of white light filaments− Properties and applications− Remote sensing of solid targets− Single and multiple filaments− White light analysis of the atmosphere− Filament-induced water condensation− Filament-based discharge control− Perspectives of lightning protection
Let‘ s propagate a millijoule femtosecondlaser pulse in air or gas!
First time observed in the lab by:
A.Braun, G.Korn, G.Mourou et al. Opt. Lett., 20(1995),73
An amazing, white-light emitting filament emerges!
E(t)Kerr:
n = n0 + n2 I(x,t)
How is the white light formed ?
E(t)( ) ( )
dt
tdIz
c
nt 02
0
ωωω −=
Self-Phase Modulation
White-Light Continuum
J.Kasparian et al., Opt. Lett. 25, 1397 (2000)
wavefront
n = n0 + n2I(r)
n2 = 3 10-19 cm2/W in air
rad
ius
ρc = 2 1021cm-3 in air
wavefront
rad
ius
Kerr Lens Plasma Lens
What is the filament formation mechanism?
c
In
ρρ )(−=∆
PropagationPropagation
Kerr Lens
Plasma
PropertiesΦ = 100 µm
L > 300 m∆n <> 10-5
Theoretical calculation
…∆n larger than thermal turbuleces -> almost no influence on propagation !
∆n <> 10-5
E = 1-5 mJI = 1014 W/cm2
ρ = 1015 cm-3
ρρρρ
Properties of these filaments
d = 100 µmL ~ 100 m, I = 1014 W/cm2,ρ = 1015 cm-3
When pumping @ 800nm
with 4mJ pulses of 60fs:
…and they areelectrically conductive!
Testing the EURO:
An emerging industrial application:*
Filament cut @ 6m distance
* Patent * Patent No.:USNo.:US 8,097,830 B28,097,830 B2
Filament Cut
An emerging medical application:
Filament cut @ 2m distanceBone and
Filament- induced breakdown spectroscopy (FIBS) on different metals
FIBS on different Minerals Future Objects
- industrial deposits
- radioactive fallouts
- mineral analysis
- radioactive fallouts
- ground humidity
- plant stress detection
But how far can we go?
Plasma-lines of copper observed at 100 meters distance
Femtosecond laser
Filament
Screen
Optimizing the supercontinuum for remote FIBS(filament induced breakdown spectroscopy)
Filament
Filterwheel
Telescope
PMT
„Signal“Genetic
algorithm
„Loop“
First preliminary results
Evolution graph
„Optimal pulse shape“ increases Supercontinuum intensity by up to
~20% compared to the optimum linear chirp.
Observations suggest:
… and now let us work at higher energies !
Mono-filamentation(<5 mJ)
Multi-filamentation(>5 mJ)
de-focussing plasma lens:
focussingKerr lens
Autoguided propagation
and multiple filamentation
At higher energies (>5 mJ): multiple filamentation
Specs of our pump laser: 240mJ @ 60fs = 4 Terawatt
And now lets produce extended filament bundles to study the atmosphere
•
Careful: Since the spectral bandwidthof our filaments is rather broad, this has to be considered,
when propagating over long distances !
400 nm 800 nmWavelenghth
fs pulse chirpedpulse
GVDno GVDcompensation
Group-Velocity Dispersion
Compensating
fs pulseanti-chirped (precompensed)
pulse
pulse
GVDwith GVDcompensation
Principle of the fs - Lidar
Chirp control
Ultrashort
Laser
Time-resolved
spectrometer
Telescope
The result:extended bundles of
FILAMENTS !
The Teramobile:A mobile fs -TW Laser and LIDAR System
Laser Titane-Saphire
Performances : 790 nm350 mJ à 10 Hz
60 fs5 TW
H. Wille et al., Eur. Phys. J. - A.P., 20, 183 (2002)J. Kasparian et al., Science 301, 61 (2003)
Tautenburg Observatorium
White Lightuntil
18 km
Positive chirp (600 fs) GVD precompensation (-600 fs)
Control of the white-light generation
Conical emission
Slight pre-compensation of GVD (-150 fs)
Ø
Ø
conical emissionh = 1900 m
White-Light Continuum
J.Kasparian et al., Opt. Lett. 25, 1397 (2000)
0.0
0.5
1.0
6800 6900 7000 7100 7200 7300 74000.0
0.5
1.0
White-light atmospheric absorption spectrum from 4 km altitude
O2
8600 8700 8800 8900 9000 9100 92000.0
0.5
1.0
8000 8100 8200 8300 8400 8500 86000.0
0.5
1.0
7400 7500 7600 7700 7800 7900 80000.0
H2O
Simultaneous oxygen and water vapor measurement
814 815 816 8170.0
0.2
0.4
0.6
0.8
1.0
1.2
Water vapor
Tra
nsm
issi
on
normalized measurement calculation
Water�Humidity
761 762 763 764 7650.0
0.2
0.4
0.6
0.8
1.0
814 815 816 817
Oxygen
Tra
nsm
issi
on
Wavelength /nm
normalized measurement calculation �Temperature
� RELATIVE humidity
Time evolution of the Ozone profile22:0
022:3
023:0
023:3
000:0
000:3
001:0
0
01:30
02:00
03:00
05:30
06:00
06:30
07:30
Ozone (µg/m3) Lyon, 29-30/07/02
What is the origin of theintensty of the observed return signals ?
Angular distribution measurementof the white-light emitted from a filament
120140160180
180 178178 176176174172 174 172
non linear 2001 linear 2001
Inte
nsi
ty (
a.u
.)
Backward enhancement of the white light emission
020406080100
threshold at 178
p_pols_polInte
nsi
ty (
a.u
.)
Angle (°)
J.Yu et al, Opt. Lett. 26(8), 533-535 (2001)
Filament-induced Condensation
P. Rohwetter et al., Nature Photonics, DOI 10.1038/NPHOTON.2010.115
Diffusion cloud chamber
fs-source:
heater
water reservoir
fs-source:800 nm, 100 fs,220 mJ
cooler
Optimization of droplet formationin th fog chambee
Laser-produced Condensation
Condensation mechanism with strong Laserlight
+
Laser
+
Fiber bundle
Laser
Filaments
Firing sequence
…
…
Δt = 1 ms T = 200 ms
Test in the real atmosphere:
The pump&probe LIDAR
Teramobile:
800nm, 220 mJ,
120 fs, 5 Hz
LIDAR transmitter:
532nm, 5 mJ, 7 ns, 10 Hz
Optical
detection
Data
Acquisition
PC
Telescope
Ref. PD
Fiber bundletime
Fiber bundle
Laser
filaments
The pump&probe LIDAR
Appearance of filament-formed droplets
Teramobile:
800nm, 220 mJ,
120 fs, 5 Hz
LIDAR transmitter:
532nm, 5 mJ, 7 ns, 10 Hz
Optical
detection
Data
Acquisition
PC
Telescope
Ref. PD
Fiber bundle
@ RH~70%!
Mark Twain (1835-1910):
« Everyone talks about the
Let´s get back to him!
« Everyone talks about the weather, but no one triesto do something about it! »
After the hail storm !
….what can be done?
Hail flyers
with Ag+I-
-
Condensation mechanism
+-
Do we want to contaminate our atmosphere wit expensiveAgI ?
Chinese bureau for weather control
Weather control
北京市人工影响天气办公室
- 37 000 employees
- 7000 rocket lounge bases
- 210 km3 rain produced (claim)
- 1/8 increase of rain (claim)
How about lightnings?
Who is threatened by lightnings?
And what can be done?
…he had the first idea!
employingrockets
A moremodernsolution :
We want to prevent this!
Remember: Filaments areelectrically conductive!
…let´s test them !
Laser guiding setup0 to —2 MV
Ground (plane electrode,Ø 3 m)
Adjustable focus
HV electrode(sphere, Ø 12 cm)
Ionized filaments
Adjustable focus
0,5 - 4 m
Contact
Laser-control of high-voltage discharges
3 m
1 MVolt 0.7 MVolt
without filament with filament
1000
1500
2000
U50
with laser U
50 without laser
Lowest LIB voltage observed
Vo
ltag
e (
kV)
Discharge triggering
0,0 0,5 1,0 1,5 2,0 2,5 3,0 3,5 4,00
500
1000
Vo
ltag
e (
kV)
D istance beween electrodes (m)
M. Rodriguez et al., Opt. Lett. 27, 772 (2002)
Filament-Triggered Discharges in RainWetting the Discharge Gap
in Rain
Filament-induced Discharge in Rain
Probability reduced by 50 %Same threshold !
Field campaignLangmuir laboratory,New Mexico TechAltitude 3200 m
Metallic hall:Faraday cage for TeramobileFaraday cage for Teramobile
Experimental Setup
filaments
E-field ?RF
RF filamentsRF
RF
Lightning Strikes
RF detectors(LMA)
Laser and filament
100 %
0 %Storm on Sept. 24/04Strong E-Field
Let us look for pulse-synchronized strikes!
Laser-controlled lightning strikes
Detectors
Laser
100 %
der Luftfahrt
98 %
Laser–inducedlightning strikes!
J. Kasparian et al., Optics Express 16, 5757 (2008)
der Luftfahrt
The future ofThe future of
lightninglightning controlcontrol
Laser
+ ++ ++
++
Laser
Thank You ! Thank You ! Thank You ! Thank You ! To the Team
MonikaPawlowska FranzHagemann PhilipRohwetter TorstenSiebert
HaoZuoquiang LW GeorgAchazi FabianWeise
MatthieuLalanne FalkoSchwaneberg AlbrechtLindinger OliverGause JörgWichmann
AndreaMerli WaltherNakaema CristinaKaposta BrigitteOdeh ThomasGelot KamilStelmaszczyk
And to our cooperation Partners:
Jean-PierreWolf JeromeKasparian