17.10.2014 Views

2.1 Ultrafast solid-state lasers - ETH - the Keller Group

2.1 Ultrafast solid-state lasers - ETH - the Keller Group

2.1 Ultrafast solid-state lasers - ETH - the Keller Group

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

124 <strong>2.1</strong>.7 Pulse characterization [Ref. p. 134<br />

<strong>2.1</strong>.7.3.2 SPIDER<br />

Spectral Phase Interferometry for Direct Electric-field Reconstruction (SPIDER) measures <strong>the</strong><br />

spectral interference of a pulse with a frequency-shifted replica [98Iac, 99Iac]:<br />

∣<br />

∣<br />

S (ω, τ) = ∣Ẽ (ω − ω 0)+Ẽ (ω − ω 0 − δω)e iωτ ∣∣<br />

2<br />

, (<strong>2.1</strong>.90)<br />

where Ẽ (ω) is <strong>the</strong> Fourier-transformation of <strong>the</strong> electric field E(t). To access <strong>the</strong> spectral phase<br />

it is necessary to produce two time-delayed replicas by a predetermined delay τ of <strong>the</strong> pulse and<br />

with a spectral shear δω between <strong>the</strong>ir carrier frequencies. The spectral shear between <strong>the</strong> central<br />

frequencies of <strong>the</strong> two replicas is generated by upconversion of <strong>the</strong> two replicas with a strongly<br />

chirped pulse using sum-frequency generation in a nonlinear optical crystal. The strongly chirped<br />

pulse is generated by propagating ano<strong>the</strong>r copy of <strong>the</strong> original pulse through a thick glass block.<br />

The spectral shear arises because <strong>the</strong> time delay between <strong>the</strong> replicas assures that each replica<br />

is upconverted with a different portion of <strong>the</strong> chirped pulse containing a different instantaneous<br />

frequency [99Gal]. The time delay τ between <strong>the</strong> replica is kept constant during <strong>the</strong> measurements<br />

and <strong>the</strong>refore only a 1D trace needs to be measured for <strong>the</strong> resulting SPIDER interferogram<br />

∣<br />

∣ ∣∣<br />

I SPIDER (ω) = ∣Ẽ(ω) 2 ∣ ∣∣ + Ẽ(ω + δω) ∣ 2<br />

∣<br />

∣<br />

∣∣<br />

+2 ∣Ẽ(ω)Ẽ(ω + δω) cos [ϕ(ω + δω) − ϕ(ω)+ωτ] . (<strong>2.1</strong>.91)<br />

The phase information can be extracted from <strong>the</strong> cosine term by <strong>the</strong> following, purely algebraic,<br />

method: The Fourier transform to <strong>the</strong> time domain of <strong>the</strong> SPIDER interferogram consists of a peak<br />

at zero time and two side peaks located near τ and −τ. The two side peaks contain equivalent phase<br />

information and are equal. One of <strong>the</strong> peaks is isolated by applying a suitable filter function and<br />

an inverse Fourier transform back to <strong>the</strong> frequency domain yields a complex function z(ω), whose<br />

complex phase gives access to <strong>the</strong> pulse spectral phase: arg (z(ω)) = ϕ(ω + δω) − ϕ(ω) +ωτ. A<br />

separate measurement of <strong>the</strong> linear phase term ωτ by spectral interferometry of <strong>the</strong> short unsheared<br />

pulse replicas is subtracted from <strong>the</strong> previous expression to yield <strong>the</strong> spectral phase difference<br />

Δϕ(ω) =ϕ(ω + δω) − ϕ(ω). From an arbitrarily chosen starting frequency ω 0 one obtains <strong>the</strong><br />

spectral phase ϕ(ω) at evenly spaced frequencies ω i = ω 0 + i · δω by <strong>the</strong> following concatenation<br />

procedure:<br />

ϕ(ω 0 )=ϕ 0 ,<br />

ϕ(ω 1 )=Δϕ(ω 0 )+ϕ(ω 0 )=ϕ(ω 0 + δω) − ϕ(ω 0 )+ϕ(ω 0 )=ϕ(ω 0 +1· δω) ,<br />

.<br />

ϕ(ω i+1 )=Δϕ(ω i )+ϕ(ω i ) .<br />

(<strong>2.1</strong>.92)<br />

The constant ϕ 0 remains undetermined but is only an offset to <strong>the</strong> spectral phase, which does not<br />

affect <strong>the</strong> temporal pulse shape and we may thus set it equal to zero. The spectral phase is written<br />

as:<br />

ϕ(ω i+1 )=<br />

i∑<br />

Δϕ(ω k ) . (<strong>2.1</strong>.93)<br />

k=0<br />

If δω is small relative to features in <strong>the</strong> spectral phase, Δϕ(ω) corresponds in first order to <strong>the</strong><br />

first derivative of <strong>the</strong> spectral phase and we can approximate <strong>the</strong> spectral phase by:<br />

ϕ(ω) ≃ 1 ∫ ω<br />

Δϕ(ω ′ )dω ′ . (<strong>2.1</strong>.94)<br />

δω ω 0<br />

The integral expression for <strong>the</strong> spectral phase has <strong>the</strong> advantage that all <strong>the</strong> measured sampling<br />

points of <strong>the</strong> interferogram can be used instead of only using a subset with sampling according<br />

Landolt-Börnstein<br />

New Series VIII/1B1

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!