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Estimation of higher order chirp in ultrashort laser pulses using modified spectrum auto-interferometric correlation

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Page 1: Estimation of higher order chirp in ultrashort laser pulses using modified spectrum auto-interferometric correlation

Optics Communications 233 (2004) 431–437

www.elsevier.com/locate/optcom

Estimation of higher order chirp in ultrashort laser pulsesusing modified spectrum auto-interferometric correlation

A.K. Sharma *, P.A. Naik, P.D. Gupta

Laser Plasma Division, Centre for Advanced Technology, Indore 452 013, India

Received 28 August 2003; received in revised form 20 January 2004; accepted 27 January 2004

Abstract

A simple method based on modified spectrum auto-interferometric correlation (MOSAIC) is presented to determine

various higher order chirps in ultrashort laser pulses. Dependence of peak amplitude and temporal shape of the locus of

the interference minima of the MOSAIC signals on different higher order chirps facilitates their determination using a

simple computer algorithm.

� 2004 Published by Elsevier B.V.

PACS: 42.65.Re

Keywords: Femtosecond laser pulse; Frequency chirp; Autocorrelation

1. Introduction

In recent years, there has been a great ad-

vancement in generation and use of ultrashort la-

ser pulses for a variety of scientific research and

applications e.g., laser matter interaction at ultra-

high intensities [1–3], high speed (terabit/s) optical

communication systems [4,5], etc. Temporal char-

acterization of these laser pulses is an important

aspect of such investigations. Simple diagnosticsystems such as single-shot second-order autocor-

relators have been reported for measurement of

* Corresponding author. Tel.: +91-7312488478; fax: +91-

7312488430.

E-mail address: [email protected] (A.K. Sharma).

0030-4018/$ - see front matter � 2004 Published by Elsevier B.V.

doi:10.1016/j.optcom.2004.01.065

pulse duration, angular chirp and resulting pulse-

front tilt of femtosecond laser beams [6–8]. De-tection and measurement of the frequency chirp in

ultrashort laser pulses is another important task as

various order chirp components produce temporal

broadening of the laser pulse. While a linear chirp

primarily increases the full width at half maximum

(FWHM) duration of the laser pulse, higher order

chirp enhances the intensity in the wings of the

laser pulse. The latter is thus a hindrance inachieving a high value of peak to pedestal intensity

contrast in the ultrashort laser pulses. Chirp may

be present in the laser pulse either due to imperfect

alignment in the compressor stage of chirped pulse

amplification (CPA) based laser systems [9] or

acquired during propagation through some dis-

persive optical components [10,11]. Diagnostics of

Page 2: Estimation of higher order chirp in ultrashort laser pulses using modified spectrum auto-interferometric correlation

432 A.K. Sharma et al. / Optics Communications 233 (2004) 431–437

the higher order chirp is therefore important for

applying necessary corrections in a laser system to

achieve desired temporal characteristics.

A variety of diagnostic tools have been devel-

oped for chirp measurements of ultrashort laser

pulses. A detailed characterization of the linear andhigher order chirp components can be carried out

using sophisticated techniques like frequency re-

solved optical gating (FROG) [12], spectral phase

interferometry for direct electrical field recon-

struction (SPIDER) [13], etc. However, these re-

quire a rather bulky experimental set-up and

involve complex numerical algorithms. On the

other hand, a detailed characterization may not benecessary in many practical situations. For exam-

ple, gross detection of the presence of chirp in a

laser pulse can be helpful in a real time optimiza-

tion of the laser system to eliminate or minimize the

chirp. In principle, interferometric auto-correlation

(IAC) [14] contains information on the chirp

present in the laser pulse. However, it does not

constitute a sensitive method for detection of chirp,especially for small magnitude of chirp. Recently,

Hirayama and Sheik-Bahae [15] proposed an in-

teresting technique of modifying the spectral con-

tents of the standard IAC signal and demonstrated

its usefulness for real time monitoring of the chirp.

The modified spectrum auto-interferometric cor-

relation (MOSAIC) signals were directly displayed

on an oscilloscope, facilitating a visual recognitionof the presence of chirp. The peak amplitude of the

locus of interference minima of the MOSAIC sig-

nals was also calculated for different values of

various order chirps for a known sech2 (t=tp) pulseshape. However, since the same peak amplitude

can be generated by several combinations of vari-

ous order chirps, this cannot be used for their un-

ambiguous quantitative determination.In this paper, we present a detailed investigation

of the characteristics of the MOSAIC signals. It is

seen that not only the peak amplitude of the locus

of the interference minima of the MOSAIC signals

but its temporal shape also depend on the mag-

nitude of different orders of chirp present in the

pulse. For instance, the temporal location of the

peak, its full width at half maximum duration, andthe asymmetry in the locus of the interference

minima of the MOSAIC signals vary differently

for different orders of the chirp and their magni-

tude. These, in turn, can be used to derive quan-

titative information on various orders of chirp.

The results are illustrated from typical examples of

MOSAIC signal computed for laser pulse with

different combinations of chirps, and deriving theinformation back using simple iterative algorithm

for a known laser pulse shape.

2. Modified spectrum auto-interferometric correla-

tion technique

The modified spectrum auto-interferometric

correlation is essentially an interferometric auto-

correlation (IAC) in which the weight factors of

different spectral components are changed to en-

hance its sensitivity for the chirp. In a second-orderautocorrelator, an ultrashort pulse laser beam is

split into two beams of equal intensity, which are

overlapped in space and time in a suitable nonlinear

medium/detector. To record the second-order in-

terferometric autocorrelation, only one fringe

should fall on the two-photon based detector.

Output of the detector as a function of time delay

between the two pulses then represents the IACsignal.

We may first examine some characteristics of the

IAC signals by considering two identical laser pulses

with their electric field amplitude given by�EðtÞ ¼ Re½EðtÞ expð�ix0tÞ�, where EðtÞ ¼ ½IðtÞ�1=2exp½i/ðtÞ�, x0 is the central frequency, IðtÞ is the

pulse intensity envelope function, and /ðtÞ is the

phase function. The latter may be expressed as

/ðtÞ ¼ aðt=tpÞ2 þ bðt=tpÞ3 þ cðt=tpÞ4; ð1Þwhere a, b and c are the magnitudes of linear,

quadratic and cubic chirps, respectively, and tp is

the FWHM duration of the laser pulse. Theoverlap intensity Iðt; sÞ as a function of the time

delay s between the two pulses would be

½EðtÞ þ Eðt � sÞ�2 i.e.,

Iðt; sÞ ¼ E2ðtÞ þ E2ðt � sÞ þ 2EðtÞEðt � sÞ cosðx0sÞ:ð2Þ

The second-order autocorrelation function,

SIACðsÞ, is then represented byRI2ðt; sÞdt, along

with the normalizing conditionRI2ðtÞdt ¼ 1, as

Page 3: Estimation of higher order chirp in ultrashort laser pulses using modified spectrum auto-interferometric correlation

A.K. Sharma et al. / Optics Communications 233 (2004) 431–437 433

SIACðsÞ ¼ 2þ 4

ZIðtÞIðt � sÞdt

þ 4

Z½IðtÞ þ Iðt � sÞ�I1=2ðtÞI1=2ðt � sÞ

� cosðx0sþ D/Þdt

þ 2

ZIðtÞIðt � sÞ cosð2x0sþ 2D/Þdt;

ð3Þ

where D/ ¼ /ðtÞ � /ðt � sÞ, is the phase differencebetween the two laser pulses.The above equation

may also be written in the form

SIACðsÞ ¼ 2þ 4G2ðsÞ þ 8F21ðsÞ cosx0s

þ 2F22ðsÞ cos 2x0s; ð4Þ

where

G2ðsÞ ¼Z

IðtÞIðt � sÞdt; ð5Þ

Normalised delay (τ/tp)-6 -4 -2 0 2 4 6

IAC

sign

al

0

4

8

12

16

Normalised delay (τ /tp)

-6 -4 -2 0 2 4 6

IAC

sign

al

0

4

8

12

16

Fig. 1. The IAC signals for no chirp (left-upper trace) and a linear c

signals are shown on the right-hand side. (A similar figure for differe

F21ðsÞ ¼ 1=2

Z½IðtÞ þ Iðt � sÞ�EðtÞE�ðt � sÞdt;

ð6Þand

F22ðsÞ ¼Z

E2ðtÞE�2ðt � sÞdt: ð7Þ

In Eq. (4), while the G2ðsÞ term, representing the

second-order intensity autocorrelation, containsinformation about the laser pulse duration, the

interference terms F21ðsÞ and F22ðsÞ are governed

by the laser pulse duration as well as the chirp

present in the pulse. However, the IAC signals are

not very sensitive to the magnitude and order of

the chirp. For instance, Fig. 1 shows the IAC

signals corresponding to no chirp condition and a

linear chirp of a ¼ 0:3 computed for a sech2 (t=tp)laser pulse. It is seen that the two signals are vi-

sually quite similar.

Normalised delay (τ/tp)-6 -4 -2 0 2 4 6

MO

SA

ICS

igna

l

2

4

6

8

10

Normalised delay (τ/tp)

-6 -4 -2 0 2 4 6

MO

SA

ICS

igna

l

2

4

6

8

10

hirp of a ¼ 0:3 (left-lower trace). The corresponding MOSAIC

nt values of the linear chirp is given by Hirayama et al. [15].)

Page 4: Estimation of higher order chirp in ultrashort laser pulses using modified spectrum auto-interferometric correlation

434 A.K. Sharma et al. / Optics Communications 233 (2004) 431–437

It is seen from Eqs. (5) and (7) that for the no

chirp condition (i.e., EðtÞ ¼ E�ðtÞ), G2ðsÞ ¼ F22ðsÞ.This fact is exploited to enhance the chirp sensi-

tivity of the IAC signals. It may be realized from

Eq. (4) that the IAC signal has three frequency

components located at dc, x0 and 2x0. The chirpsensitivity can be increased [15] by eliminating the

x0 term, amplifying the 2x0 term by a factor of 2,

and retaining the dc terms in the IAC signal. This

spectrally modified auto-interferometric correla-

tion (MOSAIC) signal is then represented as

SMOSAICðsÞ ¼ 2þ 4G2ðsÞ þ 4F22ðsÞ cos 2x0s: ð8ÞIt is easily seen from Eq. (8) that for no chirp

condition the locus of the minima of the oscil-

lating interference function SMOSAICðsÞ is a

straight line at a dc level of 2. Presence of any

chirp in the laser pulse would result in a change

in the locus of the interference minima from this

straight line. Fig. 1 shows the MOSAIC signalscomputed for the no chirp condition and for a

linear chirp of a ¼ 0:3, for a sech2 (t=tp) pulse.

This is similar to Fig. 1 shown in work of Hi-

rayama et al. [15] for a linear chirp of 0.15 and

0.25 to illustrate the MOSAIC technique. A clear

difference in the locus of interference minima is

observed for the chirp case, which shows two

peaks symmetrically located about the zero timedelay. Occurrence of such peaks, henceforth re-

ferred to as MOSAIC peaks, facilitates visual

detection of the chirp.

Normalized mean chirp

0.0 0.2 0.4 0.6 0.8 1.0

Nor

mal

ised

ampl

itude

ofM

OS

AIC

peak

0.00

0.05

0.10

0.15

0.20

0.25

0.30

Linear chirp

Cubic chirp

Quadratic chirp

Fig. 2. Dependence of the normalized amplitude of MOSAIC

peak on the normalized mean chirp for linear, quadratic and

cubic chirps. (This figure has been adapted from the work of

Hirayama et al. [15].)

3. Dependence of the MOSAIC signal on the chirp

parameters

Eqs. (4)–(7) reveal that the peak amplitudes of

the loci of interference maxima and minima of the

MOSAIC signals will depend on the magnitude

and order of the chirp. Moreover, the two loci

have a common dc background of 2. We therefore

define normalized peak amplitude of the MOSAIC

signal as the ratio of peak amplitude of the locus

of minima to that of maxima, after subtracting thedc background. In general, this normalized peak

amplitude increases with increasing magnitude of

the chirp. Further, in order to facilitate compari-

son of the results for different orders of the chirp,

we use normalized mean chirp (NMC) parameter

[15] (weighted over the laser pulse shape) as

NMC ¼Z

IðtÞ t0d/dt

��������dt

ZIðtÞdt

�: ð9Þ

The normalized peak amplitude of the MOSAIC

signal was computed for different values of NMCfor linear, quadratic and cubic chirps for a sech2

(t=tp) pulse. Fig. 2 shows the dependence of the

normalized peak amplitude on the NMC in the

range from 0 to 1 rad. This figure has been adapted

from the work of Hirayama et al. [15] to facilitate

extension of MOSAIC technique to determine

various order chirps. It is seen that the MOSAIC

peak varies differently for different orders of chirp.It may be observed that a small amplitude of the

MOSAIC peak does not necessarily mean a neg-

ligible chirp because higher order chirps with large

values of NMC may be present. Further, it is no-

ted from Fig. 2 that a given peak amplitude of the

MOSAIC signal can occur for several different

combinations of various order chirps. For illus-

tration, Fig. 3 shows the loci of interference min-ima of the MOSAIC signal for two different chirp

conditions viz. (a) quadratic chirp of b � 0:17(NMC¼ 0.43) and (b) cubic chirp of c � 0:05(NMC¼ 0.28). The normalized peak amplitudes of

the MOSAIC signals in the two cases are same

(equal to 0.05). The same situation also occurs for

Page 5: Estimation of higher order chirp in ultrashort laser pulses using modified spectrum auto-interferometric correlation

Normalised mean chirp0.2 0.4 0.6 0.8 1.0

Tem

pora

lasy

met

rypa

ram

eter

(∆t

2/∆t

1)

0.8

0.9

1.0

1.1

1.2

1.3

1.4

1.5

1.6

Cubic chirp

Linear chirp

Quadratic chirp

Fig. 5. The temporal asymmetry parameter of the MOSAIC

signal for different values of the normalized mean chirp for

linear, quadratic, and cubic chirps.

Temporal delay (τ/tp)

-5 -4 -3 -2 -1 0 1 2 3 4 5Nor

mal

ised

ampl

itude

ofin

terf

eren

cem

inim

a

0.00

0.02

0.04

0.06

0.08

Quadratic chirp[β γ~ 0.17 (NMC ~ 0.43)]

Cubic chirp [ ~ 0.05 (NMC ~ 0.28)]

∆t1 ∆t2

Fig. 3. Loci of the interference minima of the MOSAIC signal

for two different chirp conditions are shown: (a) quadratic chirp

b � 0:17, NMC¼ 0.43 (solid line); (b) cubic chirp c � 0:05,

NMC¼ 0.28 (dotted line). The amplitudes of the MOSAIC

peaks are equal in the two cases.

Normalised mean chirp0.0 0.2 0.4 0.6 0.8 1.0

Tem

pora

lloc

atio

nof

MO

SA

ICP

eak

[ τ/t p]

1.0

1.5

2.0

2.5

3.0

Linear chirp

Quadratic chirp

Cubic chirp

Fig. 4. Variation of the temporal location of the MOSAIC

peak with normalized mean chirp for linear, quadratic, and

cubic chirps.

A.K. Sharma et al. / Optics Communications 233 (2004) 431–437 435

a linear chirp of a � 0:17 (NMC¼ 0.24). Thus a

knowledge of the normalized peak amplitude of

the MOSAIC signal alone can not predict the

magnitude and order of the different chirps.

Next, we examine the dependence of temporalshape of the MOSAIC peak on the chirp param-

eters. For instance, one may note from Fig. 3 that

the temporal location of the MOSAIC peak is

different for the two chirp conditions shown. It is

also observed from Fig. 3 that the MOSAIC sig-

nals are asymmetric with respect to the temporal

location of the peak. This asymmetry is more ev-

ident for the case of quadratic chirp. The temporalfeatures of the MOSAIC peak may be broadly

expressed in terms of: (1) the location of the peak

(2) the FWHM duration and (3) the asymmetry

parameter. The last one may be defined as ratio of

the two half widths at half maximum i.e., Dt2=Dt1as depicted in Fig. 3. Dependence of the temporal

location of the peak on the normalized mean chirp

computed for linear, quadratic and cubic chirpsfor sech2 (t=tp) pulse is shown in Fig. 4. It is seen

that, for all the three cases, the peak time decreases

with increase in magnitude of the chirp. Further, it

is observed from Fig. 4 that for cubic chirp the

peak of MOSAIC signal occurs at a much larger

time delay as compared to that for linear and

quadratic chirps.

Figs. 5 and 6 show the temporal asymmetry

parameter (Dt2=Dt1) and the FWHM duration of

the MOSAIC signal, respectively, as a function of

the normalized mean chirp for linear, quadratic

and cubic chirp. It is interesting to note that in

presence of cubic chirp, the MOSAIC signal re-mains almost symmetric with respect to its peak in

contrast to the asymmetric profiles for linear and

quadratic chirps. This may be useful as a visual

indicator of the presence of cubic chirp. Next, the

FWHM duration of the MOSAIC signal (Fig. 6)

decreases with increasing magnitude of the chirp.

This decrease is more steep for linear chirp as

Page 6: Estimation of higher order chirp in ultrashort laser pulses using modified spectrum auto-interferometric correlation

Normalised mean chirp0.0 0.2 0.4 0.6 0.8 1.0F

WH

Mdu

ratio

n[( ∆

t 1+∆t

2)/t

p]of

MO

SA

ICpe

ak

1.4

1.6

1.8

2.0

2.2

2.4

2.6

2.8

Quadratic chirp

Linear chirpCubic chirp

Fig. 6. FWHM duration of the MOSAIC signal for different

values of the normalized mean chirp for linear, quadratic and

cubic chirps.

436 A.K. Sharma et al. / Optics Communications 233 (2004) 431–437

compared to that for the quadratic and cubic

chirps.

4. Determination of the chirp parameters from the

MOSAIC signals

Different dependences of the peak amplitude

and temporal characteristics of the MOSAIC sig-

nal on the magnitude and order of the chirp pre-

sented above may be used for quantitativeestimation of the chirp parameters. In many

practical situations such as chirp pulse amplifica-

tion based laser systems, the linear chirp can be

easily eliminated/minimized. Detection of any

quadratic and cubic chirp from the MOSAIC sig-

nals in this case becomes much easier because for

an observed amplitude of the MOSAIC peak, the

temporal location (Fig. 4) and the asymmetry pa-rameter (Fig. 5) are quite different for the two

cases. In general, various order chirp components

may be simultaneously present in the laser pulse so

that the amplitude and temporal characteristic of

the MOSAIC peak may not conform to any par-

ticular order. Here the chirp parameters can be

determined by matching the observed MOSAIC

signals with the computed ones through an itera-tive procedure for various combinations of differ-

ent order phase terms involving a, b and c.The task of iterative fitting of MOSAIC signals

gets much simplified by putting conditions of

minimum and maximum on the values of NMC.

The latter are identified from the observed values

of peak amplitude and temporal location of the

MOSAIC peak. From Fig. 2, it is clear that the

amplitude of the MOSAIC peak increases with

increase in the NMC for all chirp orders. This putsa lower limiting value on the normalized mean

chirp, NMCmin, which is the smallest of the NMC

values corresponding to the observed value of the

normalized peak amplitude for different chirp or-

ders. Similarly, Fig. 4 shows a decreasing behavior

for the time of occurrence of the MOSAIC peak

with increasing NMC for all chirp orders. This, in

turn, puts an upper limiting value on the normal-ized mean chirp, NMCmax, which is the largest of

the NMC values corresponding to the observed

value of the time of occurrence of the MOSAIC

peak for different chirp orders. The actual NMC

for the given MOSAIC signal should lie between

NMCmin and NMCmax.

A simple computer program has been written to

find out the values of the chirp parameters a, b andc from the given IAC signal. Firstly, the observed

IAC signal is converted into MOSAIC signal by

carrying out the following steps: (a) the IAC signal

is decomposed into its Fourier components using

fast Fourier transform algorithm, (b) the 2x0

component is multiplied by a factor of 2 and the

same is added to the dc term, and finally (c) by

using inverse fast Fourier transform, the modifiedsignal in frequency domain is converted into time

domain to get the MOSAIC signal i.e., SMOSAICðsÞ.Next, the program generates various possible

combinations of a, b and c which have NMC in the

range NMCmin to NMCmax. In the present exercise,

the step size was taken to be Da ¼ 0:05, Db ¼ 0:02and Dc ¼ 0:01. The program then computes MO-

SAIC signals for a sech2 (t=tp) laser pulse andcompares them with the given MOSAIC signal.

The computed MOSAIC signal with minimum

value of rms error (with respect to the reference

MOSAIC signal) was identified, and the corre-

sponding values of a, b and c give the chirp pa-

rameters. This procedure was tested on a number

of pre-calculated MOSAIC signals for different

combinations of a, b and c. For example a MO-SAIC signal was computed for a ¼ 0:2(NMC� 0.28), b ¼ 0:06 (NMC� 0.15), and

Page 7: Estimation of higher order chirp in ultrashort laser pulses using modified spectrum auto-interferometric correlation

A.K. Sharma et al. / Optics Communications 233 (2004) 431–437 437

c ¼ 0:04 (NMC� 0.22). It had a normalized peak

amplitude of 0.10, temporal location of the peak

s=tp ¼ �1:6, and asymmetry parameter Dt2=Dt1 ¼1:19 (Dt2 ¼ 1:00tp and Dt1 ¼ 0:84tp). The lower andupper limiting values of NMC for the above am-

plitude and temporal location of the peak wereNMCmin ¼ 0.39 and NMCmax ¼ 0.91. It was possi-

ble to get back the original values of a, b and cwithin the step accuracy. Moreover, this determi-

nation was not sensitive to a random noise of �5%

imposed on the MOSAIC signal.

In conclusion, we have presented a simple

method of quantitative estimation of linear and

higher order chirps based on analysis of themodified spectrum auto-interferometric correla-

tion (MOSAIC) signals. It is shown that the peak

amplitude, the temporal location of the peak, the

FWHM duration, and the asymmetry of the locus

of the interference minima exhibit different de-

pendences on magnitude of the chirp and its order.

These, in turn, facilitate diagnostic of the chirp

parameters of ultrashort laser pulses through aFourier transform based computer algorithm. The

method is particularly suited to determine small

values of higher order chirps in ultrashort laser

pulses.

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