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Page 1: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation
Page 2: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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

Page 3: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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

Page 4: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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!

Page 5: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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

Page 6: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

White-Light Continuum

J.Kasparian et al., Opt. Lett. 25, 1397 (2000)

Page 7: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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

Page 8: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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

Page 9: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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:

Page 10: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

…and they areelectrically conductive!

Page 11: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Testing the EURO:

Page 12: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

An emerging industrial application:*

Filament cut @ 6m distance

* Patent * Patent No.:USNo.:US 8,097,830 B28,097,830 B2

Page 13: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Filament Cut

Page 14: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

An emerging medical application:

Filament cut @ 2m distanceBone and

Page 15: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Filament- induced breakdown spectroscopy (FIBS) on different metals

Page 16: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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?

Page 17: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Plasma-lines of copper observed at 100 meters distance

Page 18: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Femtosecond laser

Filament

Screen

Optimizing the supercontinuum for remote FIBS(filament induced breakdown spectroscopy)

Filament

Filterwheel

Telescope

PMT

„Signal“Genetic

algorithm

„Loop“

Page 19: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

First preliminary results

Evolution graph

Page 20: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

„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 !

Page 21: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Mono-filamentation(<5 mJ)

Page 22: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Multi-filamentation(>5 mJ)

Page 23: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

de-focussing plasma lens:

focussingKerr lens

Autoguided propagation

and multiple filamentation

At higher energies (>5 mJ): multiple filamentation

Page 24: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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

Page 25: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

fs pulse chirpedpulse

GVDno GVDcompensation

Group-Velocity Dispersion

Compensating

fs pulseanti-chirped (precompensed)

pulse

pulse

GVDwith GVDcompensation

Page 26: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Principle of the fs - Lidar

Chirp control

Ultrashort

Laser

Time-resolved

spectrometer

Telescope

Page 27: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

The result:extended bundles of

FILAMENTS !

Page 28: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

The Teramobile:A mobile fs -TW Laser and LIDAR System

Page 29: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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)

Page 30: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Tautenburg Observatorium

Page 31: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

White Lightuntil

18 km

Page 32: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Positive chirp (600 fs) GVD precompensation (-600 fs)

Control of the white-light generation

Page 33: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Conical emission

Slight pre-compensation of GVD (-150 fs)

Ø

Ø

conical emissionh = 1900 m

Page 34: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

White-Light Continuum

J.Kasparian et al., Opt. Lett. 25, 1397 (2000)

Page 35: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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

Page 36: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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

Page 37: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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

Page 38: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

What is the origin of theintensty of the observed return signals ?

Angular distribution measurementof the white-light emitted from a filament

Page 39: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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)

Page 40: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Filament-induced Condensation

P. Rohwetter et al., Nature Photonics, DOI 10.1038/NPHOTON.2010.115

Page 41: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Diffusion cloud chamber

fs-source:

heater

water reservoir

fs-source:800 nm, 100 fs,220 mJ

cooler

Page 42: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Optimization of droplet formationin th fog chambee

Page 43: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Laser-produced Condensation

Page 44: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Condensation mechanism with strong Laserlight

+

Laser

+

Page 45: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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

Page 46: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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%!

Page 47: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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! »

Page 48: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation
Page 49: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

After the hail storm !

….what can be done?

Page 50: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Hail flyers

Page 51: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

with Ag+I-

-

Condensation mechanism

+-

Do we want to contaminate our atmosphere wit expensiveAgI ?

Page 52: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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)

Page 53: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

How about lightnings?

Page 54: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Who is threatened by lightnings?

And what can be done?

Page 55: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

…he had the first idea!

Page 56: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

employingrockets

A moremodernsolution :

Page 57: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

We want to prevent this!

Page 58: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Remember: Filaments areelectrically conductive!

…let´s test them !

Page 59: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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

Page 60: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Laser-control of high-voltage discharges

3 m

Page 61: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

1 MVolt 0.7 MVolt

without filament with filament

Page 62: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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)

Page 63: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Filament-Triggered Discharges in RainWetting the Discharge Gap

in Rain

Page 64: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Filament-induced Discharge in Rain

Probability reduced by 50 %Same threshold !

Page 65: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Field campaignLangmuir laboratory,New Mexico TechAltitude 3200 m

Metallic hall:Faraday cage for TeramobileFaraday cage for Teramobile

Page 66: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Experimental Setup

filaments

E-field ?RF

RF filamentsRF

RF

Page 67: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Lightning Strikes

RF detectors(LMA)

Laser and filament

100 %

0 %Storm on Sept. 24/04Strong E-Field

Let us look for pulse-synchronized strikes!

Page 68: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

Laser-controlled lightning strikes

Detectors

Laser

100 %

der Luftfahrt

98 %

Laser–inducedlightning strikes!

J. Kasparian et al., Optics Express 16, 5757 (2008)

der Luftfahrt

Page 69: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

The future ofThe future of

lightninglightning controlcontrol

Laser

+ ++ ++

++

Laser

Page 70: Fundamentals and Applications of - · PDF fileJ. Kasparian et al. , Science 301 , 61 (2003) Tautenburg Observatorium. White Light until 18 km. Positive chirp (600 fs) GVD precompensation

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