Wavelength Tunable Passively Q-Switched Alexandrite Laser with
Direct Diode-Pumping at 635 nm
Ufuk Parali
1,2*
, Gabrielle M. Thomas
1
, Ara Minassian
3
, Xin Sheng
1
and Michael J. Damzen
1
1
Photonics Group, The Blackett Laboratory, Imperial College London, London, SW7 2AZ, U.K.
2
Department of Computer Engineering, Adnan Menderes University, Aydin, 09010, Turkey
3
Unilase Ltd, 1 Filament Walk, Unit G02, London, SW18 4GQ, U.K.
Keywords: Alexandrite, Passive Q-Switch Lasers, Tunable Lasers, Diode-Pumped Lasers.
Abstract: We report on a wavelength tunable passively Q-switched Alexandrite laser directly red-diode-pumped at
635 nm. Passive Q-switching was achieved with a semiconductor saturable absorber mirror (SESAM) and
wavelength tuning with a birefringent tuner. The pulse repetiton rate was variable on the pump power and
wavelength and a maximum 27 kHz rate was achieved in fundamental TEM
00
mode. The maximum average
output power obtained was 41 mW. The Q-switched wavelength tuning band was studied between 740 nm
and 755 nm. To the best of our knowledge, this is the first time that tunable TEM
00
passive Q-switched
operation of a diode-pumped Alexandrite laser has been achieved. The results obtained in this study can be
significantly further optimised for performance. A new cavity configuration for this optimisation is
described. Future work is expected to lead to the development of higher power, more efficient tunable
passive Q-switched (and potentially passive mode-locked) diode-pumped Alexandrite laser sources in the
near-infrared band and also ultraviolet region through frequency conversion.
1 INTRODUCTION
Laser sources possessing broad emission bandwidths
can provide wavelength tunable in a wide range with
capability of different pulse durations (ns/ps/fs) and
capability to potentially offer significantly benefit to
many technological and scientific studies. Nonlinear
microscopy, optical coherence tomography,
frequency conversion, generation of high power
ultrashort optical pulses and remote sensing
applications can be given as some examples
(Damzen, 2014; Teppitaksak, 2014; Koechner,
2003; Ghanbari, 2016;). In air-borne (and also in
space-borne) remote sensing with laser-based lidar
and altimetry techniques, such as resonant
backscatter lidar, ground vegetation bio-mass/bio-
health detection etc., such laser sources could
provide a powerful tool for 3-D mapping of
atmospheric species and physical attributes, spectral
indicators of Earth features and high precision
ground topography (Damzen, 2014; Eitel, 2011; Lu,
2016; Pelon, 1986; Milton, 1997; Chen, 2014). This
would provide a valuable source for understanding
the atmospheric science and health of the Earth
vegetation and ecological system (Eitel, 2011).
However, these remote sensing techniques requires
the utilization of cutting-edge laser technologies
having space-borne qualification. The exacting
requirements for spaceborne operation severely
restricts the class of lasers compatible in the space
environment. The primary laser system with long
space heritage is the diode-pumped Nd:YAG laser
(Damzen, 2014; Eitel, 2011). However, this laser
system has narrow linewidth and does not allow for
wavelength tunability providing only a discrete
single frequency at its primary fundamental laser
line 1064 nm and its higher harmonics at 532 nm
and 355 nm. Thus, accessing other wavelength
regions at these systems is only possible by optical
parametric conversion methods leading to higher
complexity and cost and lower reliability and
efficiency (Teppitaksak, 2014; Koechner, 2003;
Ghanbari, 2016; Teppitaksak, 2015). An alternative
approach for obtaining wavelength tunability and
pulse generation capabilities by directly diode laser
pumping is the utilization of vibronic solid-state
laser materials. Today, the most commonly used
vibronic laser systems are Ti:Sapphire solid-state
lasers, which have the broadest gain bandwidth
permitting direct generation of a few cycle optical
82
Parali U., Thomas G., Minassian A., Sheng X. and Damzen M.
Wavelength Tunable Passively Q-Switched Alexandrite Laser with Direct Diode-Pumping at 635 nm.
DOI: 10.5220/0006155500820089
In Proceedings of the 5th International Conference on Photonics, Optics and Laser Technology (PHOTOPTICS 2017), pages 82-89
ISBN: 978-989-758-223-3
Copyright
c
2017 by SCITEPRESS Science and Technology Publications, Lda. All rights reserved
pulses (Teppitaksak, 2014; Koechner, 2003;
Ghanbari, 2016; Beyatli, 2013; Demirbas, 2009).
However, these lasers usually requires complex
pump sources causing disadvantages such as
complex system structure, bulky and large physical
size, and low efficiency of electrical-optical
conversion (Teppitaksak, 2014; Demirbas ,2009). As
an alternative class of vibronic laser crystals, there
are the well-known Cr-doped colquiriites
(Cr:LiSAF, Cr:LiCAF and Cr:LiSGaF) and Cr-
doped chrysoberyl (Cr:BeAl
2
O
4
) more commonly
known as Alexandrite (Teppitaksak, 2014; Ghanbari,
2016; Beyatli, 2013; Sennaroglu, 1998; Demirbas,
2009; Sennaroglu, 2007). Among these crystals,
however there are some performance-limiting
disadvantages such as upper-state lifetime quenching
at elevated temperatures, poor thermal conductivity
and excited state absorption, Cr-doped colquiriite
lasers are not attractive alternatives (Koechner,
2003; Ghanbari, 2016). Conversely, Alexandrite has
a number of superior optical and thermo-mechanical
properties making it an attractive vibronic solid-state
laser gain medium. Alexandrite can be direct diode-
pumped by red, green and blue laser diodes due to
its broad absorption bands in the visible range
(Koechner, 2003; Ghanbari, 2016). However for
highest efficiency and lowest heating factor the red
diodes provide the most favourable pump sources. It
has a fracture resistance five-times bigger than that
of Nd:YAG. And its thermal conductivity (23Wm
-
1
K
-1
) (Koechner, 2003) is almost twice that of
Nd:YAG and five-times that of the Cr doped
colquiriites. The laser emission of the Alexandrite is
highly linearly polarized due to the birefringence of
the crystall eliminating the depolarization problems
(Teppitaksak, 2014; Koechner, 2003). Its relatively
longer upper-state lifetime (~260μs) at room-
temperature provides a good energy storage
potential for Q-switched operation (Teppitaksak,
2014). Moreover, Alexandrite’s laser performance is
increased at elevated temperatures due to its unique
spectroscopic properties (Loiko, 2016). It has a
relatively low stimulated emission cross section (0.7
× 10
-20
cm
2
) requiring intense diode pumping
(Koechner, 2003). Historically, it is the first
wavelength tunable solid state laser operated at room
temperature. Alexandrite has a broad emission
wavelength range from ~ 700 nm to 850 nm
(Walling, 1985; Sam, 1980). This spectral band is
especially important. It is in the biological window
for tissue transmission and for remote sensing of
vegetation sits across the so-called red-edge band
(~700-750nm) of chlorophyll (Eitel, 2011). This
band is the steep rising transition band between high
red and visible absorption and high near-IR
reflection. Changes in this spectral band are well-
known as indicators of plant health (Eitel, 2011). It
is very interesting for a vegetation lidar to have a
laser with emission wavelength range covering this
red-edge band range.
Recently, in our prior work at Imperial College,
continuous-wave (cw) red diode-pumped
Alexandrite laser with 26W of average output power
was obtained and the first active Q-swithcing with
an electro-optic Pockels cell (Teppitaksak, 2014).
Interestingly, the first femtosecond Kerr-lens mode-
locked Alexandrite laser was recently reported in
(Ghanbari,2016) producing pulses as short as 170 fs.
In this study, we report the first successfully
demonstration of a wavelength tunable passive Q-
switched Alexandrite laser with semiconductor
saturable absorber mirror (SESAM) and using a red
diode (AlGaInP) pump laser at 635 nm. For tuning
the wavelength, a birefringent filter (BiFi) was used
in the cavity. The highest repetiton rate achieved
was 27 kHz in fundamental TEM
00
mode. The
maximum average output power obtained was 41
mW. The shortest pulse generated was 550 ns
(FWHM). The wavelength tuning band spanned was
between 740 nm and 755 nm. To the best of our
knowledge, this is the first wavelength tunable
TEM
00
passive Q-switched operation of a red diode-
pumped Alexandrite laser. Our results open the way
for further development, optimization and power
scaling of this new generation passive Q-switched
(and also potentially for passive mode-locked)
Alexandrite lasers. One interesting application for
developing a low-cost, compact and wavelength
tunable pulsed laser source is space-borne remote
sensing applications, especially for the next
generation vegetation lidar systems.
2 EXPERIMENTAL SETUP
A simple linear cavity was designed to study the
wavelength tunable passive Q-switching operation
mode of the direct diode-pumped Alexandrite laser.
Two experimental systems are described. The first is
a wavelength tunable cw setup shown in Figure 1 as
a precursor study. The second setup was a
wavelength tunable passive Q-switched using a
semiconductor saturable absorber mirror (SESAM)
as shown in Figure 2.
The wavelength tunable cw laser had a plane-plane
mirror cavity. The Alexandrite gain medium was a
10 mm-long and 4 mm-diameter Alexandrite rod
crystal doped with 0.22% of Cr
3+
and c-axis cut. The
Wavelength Tunable Passively Q-Switched Alexandrite Laser with Direct Diode-Pumping at 635 nm
83
Figure 1: Schematic layout of the plane-plane mirror cavity wavelength tunable continuous-wave direct red diode-pumped
Alexandrite laser operating in fundamental TEM
00
mode.
Figure 2: Schematic layout of the wavelength tunable passive Q-switched direct red diode-pumped Alexandrite laser. Here,
OC in Figure 1 is replaced with SESAM. The output coupling is provided from the reflection of the BiFi in the cavity.
end faces of the rod were plane-parallel and anti-
reflection coated at the Alexandrite wavelength
(~755 nm). The rod was mounted in water-cooled
copper heat-sink and an indium foil interface used
for enhanced thermal contacting to the copper.
The cavity length ~142 mm including an intracavity
plano-convex lens (PCX, f=70 mm). The intracavity
lens design was chosen to form a stable cavity
configuration and to optimise for TEM
00
operation.
A dichroic back mirror (BM) was highly-reflecting
(R>99.9%) at laser wavelength (~755nm) and
highly-transmitting (R<0.2%) for pump diode laser
(~635 nm). Both the temperature of the crystal and
pump laser diode were cooled to 16
o
C using a
single water chiller in the experiments.
The small-signal absorption coefficient (α) of the
crystal measured ~6cm
-1
with a He-Ne laser at 633
nm for light polarized parallel to the b-axis of
Alexandrite crystal. The crystal was pumped by a
red diode module, operating nominally at central
wavelength 635nm with bandwidth (FWHM) of ~
1.5nm and capable of providing max ~5W (5180
mW full power) in cw mode. The diode module is
fibre coupled in a multi-mode fiber with core
diameter of 105 µm and numerical aperture of 0.22.
An aspheric fiber collimator with 35mm of focal
length was used for collimating the pump beam
output from the fiber. The circularized pump beam
was focused into a ~120 μm spot size diameter
inside the crystal by an aspheric pump lens (ASP) of
50 mm focal length.
The output of the fibre was not a pure polarisation
but > 60% was in the highly absorbing b-axis
direction of the Alexandrite crystal. About 83% of
the pump power was absorbed in the crystal. The
confocal parameter of the b-axis component of the
pump (~4 mm) was sufficiently longer than the
absorption depth of the crystal to allow good laser
mode overlap with the pump. The overlap of the
laser mode to the other polarisation however would
be poor.
The wavelength tuning of the laser is provided by
using a quartz plate with a thickness of 0.5 mm
acting a birefringent filter (BiFi) tuner. The BiFi sits
at Brewster angle (to minimize insertion losses) and
wavelength tuned by rotation of the BiFi in the plane
of the plate using a goniometer to alter the
birefringence of the plate. In this way it was simple
to tune the wavelength of the laser output of both
cavities (Figures 1 and 2) working in cw and passive
Q-switched mode.
For optimizing the laser cavity and as a reference,
we first obtained the cw mode of operation by using
an output coupler (OC) with 99.5% reflectivity
(Figure 1). The output of the wavelength tunable
cavity working in cw mode is obtained through the
65 mm
75 mm
BiFi
Fibre
collimator
50 mm
5W
fibre coupled
red diode
λ/2
waveplate
ASP=
50mm
Crystal
0.22%
PCX=70m
SESAM
2.5 mm
Output
Bea
m
Dichroic
BM
70 mm
70 mm
BiFi
Fibre
collimator
50 mm
5W
fibre coupled
red diode
λ/2
waveplate
ASP=
50mm
Dichroic
BM
PCX=70mm
OC
99.5%
2 mm
Crystal
0.22%
Output
Bea
m
PHOTOPTICS 2017 - 5th International Conference on Photonics, Optics and Laser Technology
84
OC. Once the cavity was optimized in cw mode, we
replaced the OC with a SESAM to obtain passive Q-
switching mode (Figure 2). The output beam was
obtained from the BiFi since the SESAM was used
as the end mirror in the cavity and was non-
transmitting as it was attached on an aluminium disc
using thermal adhesive. This helped to increase the
heat transfer between SESAM and the aluminum.
The beam spot size diameter on the SESAM was
calculated about to be ~250 µm. The SESAM had a
saturable absorption with modulation depth ~ 0.5%
and had also some nonsaturable loss (~1%). Both the
nonsaturable loss and modulation depth depends on
wavelength. The SESAM structure had a ~60 nm
reflectivity bandwidth centered around 740 nm
(R=~99%) and a ~10 nm (FWHM)
photoluminescence band centered around ~736 nm.
The dynamic response (absorption recovery) of the
SESAM was biexponential with <0.5 ps for fast
component and ~300 ps for slow component. The
saturation intensity was around ~30 µJ/cm
2
.
3 RESULTS AND DISCUSSION
In the initial experiments, we investigated the
variation of the cw output power as a function of
emission wavelength. The wavelength of the
Alexandrite laser with the 99.5% reflectivity output
coupler was tuned in the range extended from 730
nm to 790 nm and the output power shown in
Figure 3. Maximum output power was obtained at
740 nm lasing wavelength at full pump power ~5W
(5180 mW) at 635 nm. It can be seen from Fig.3 that
a much wider tuning range was possible, however
the main focus of this study was operation around
the wavelength band of the SESAM device.
Figure 3: Tuning curve for the cw Alexandrite laser with
0.5 mm BiFi tuner plate. Alexandrite crystal temperature
was 16
o
C, output coupler was 0.5% transmitting, and
incident pump power was 5180 mW.
By fixing the angle of the BiFi so that the laser
output wavelength is constant at 740 nm, the
measured cw output power versus the pump power
curve of the cavity is depicted in Figure 4. The slope
efficiency was ~14% and shows no sign of
decreasing at the highest output power. This
suggests that thermal lensing effects did not limit the
output power. As can be further seen in Figure 4, the
slope efficiency and output power is increasing with
the available pump power, suggesting that the power
performance can be further improved with more
powerful pump lasers. The optical-to-optical
efficiency with respect to incident pump power can
also be expected to be considerably increased by
optimising output coupling, reducing intracavity loss
and attention to spectral profile of coated cavity
optics.
Figure 4: Output power vs Pump power curve of cw
Alexandrite laser cavity at constant wavelength of λ=740
nm. Laser crystal is at 16
o
C and 0.5% transmitting output
coupler.
After the characterisation of the wavelength tunable
cw laser cavity, the OC mirror was replaced with the
SESAM for passively Q-switching the Alexandrite
laser. The output of the laser was provided by a
reflection loss from the BiFi plate. With the
dimensions of the cavity as shown in Figure 2, the
system started working in a self-Q-switched mode.
In particular, after the alignment of the cavity was
optimized, the output power showed a strong
dependence on the position of the intracavity lens
that might be to do the spot size on the SESAM.
For constant wavelength λ=747 nm (by fixing the
BiFi at appropriate angle), the evolution of the
output power, pulse width and the repetiton rate with
respect to the pump power are given in Figure 5. It
is noted that the cavity has a higher threshold due to
the larger losses incurred by insertion of the
SESAM. As the available pump power increases
730 740 750 760 770 780 790
120
140
160
180
200
220
240
Wavelength (nm)
Output Power (mW)
Output characteristics of wavelength tunable
cw Alexandrite laser direct diode-pumped at 635 nm
Output Pow er (mW) at 5180 mW
full pump power
2000 2500 3000 3500 4000 4500 5000 5500
0
50
100
150
200
250
Pump Power (mW)
Output Power (mW)
Output characteristics of wavelength tunable
cw Alexandrite laser direct diode-pumped at 635 nm
cw output power (mW) at 740 nm
Wavelength Tunable Passively Q-Switched Alexandrite Laser with Direct Diode-Pumping at 635 nm
85
above threshold, shorter pulses with higher
repetition rate were obtained.
Figure 5: For constant wavelength λ=747 nm, the
evolution of the output power, pulse width and the
repetiton rate of the passive Q-switched diode-pumped
Alexandrite laser with respect to the 635 nm pump power.
The slope efficiency was limited by the intracavity
losses and can be improved by careful intracavity
loss management. Moreover, the output is obtained
from the BiFi in the cavity meaning that the actual
power generated by the cavity is higher than the
measured value. Although this is not the best
configuration for obtaining the output pulse from a
laser cavity, we preferred to use this cavity
configuration as shown in Figure 2. Our objective in
choosing this setup was to make the system as
simpler as possible in order to just show
experimentally for the first time that the diode-
pumped Alexandrite crystal can be passively Q-
switched. In our future studies, we are planning to
use an X-Cavity (as described in Section 4) and/or
L-cavity configurations with higher crystal
temperature to obtain higher efficiency and higher
pump power to provide higher output power in
passive Q-switching of diode-pumped Alexandrite
laser.
In the tunable passive Q-switching experiments, the
BiFi was again used to tune the wavelength but was
also restricted by the limited reflectivity band of the
SESAM and range over which Q-switching could be
accomplished. The tuning bandwidth achieved was
between 740 nm and 755 nm (Figure 6). Compared
with the cw tuning range shown in Figure 3, Q-
switching tuning bandwidth is narrower. Figure 6
shows the evolution of the output power, pulse
width, repetition rate and spectral width of the pulses
obtained from the passive Q-switched diode-pumped
Alexandrite laser in the wavelength tunability range
for full pump power.
Figure 6: The output power, pulse width, repetition rate
and spectral width of the pulses obtained in the
wavelength tunability range from the passive Q-switched
Alexandrite laser.
The highest pulse repetition rate was 27 kHz at 755
nm and the shortest pulse width was 550 ns at 740
nm. The observed spectral width was <1 nm for the
tuning range of the passive Q-switch mode. Figure 7
compares the pulse widths and spatial profiles
obtained at the wavelengths 743 nm and 750 nm for
full pump power. The laser output beams for both
wavelengths had TEM
00
beam profile with M
2
values
<1.7 and <1.9 for 743 nm and 750 nm, respectively.
The M
2
beam quality was determined using the ISO
11146-1 method, based on the second moment beam
size. When the mode of the beam profile was
adjusted to higher spatial modes, higher output
power was achieved due to the increased mode-gain
overlap in the cavity.
Figure 7: Pulse profiles and spatial profiles obtained at
743 nm and 750 nm from the tunable passive Q-switched
Alexandrite laser.
Figure 8 shows the pulse train and the repetition
rates obtained at the wavelengths 743 nm and 750
nm for full pump power. At 743 nm a pulse
repetition rate of 14 kHz was obtained, whilst at 750
nm the repetition rate was higher at 23 kHz.
A photograph of the developed laser is shown in
Figure 9 below (see Figure 2 for dimensions and
600
800
1000
1200
1400
1600
1800
2000
Pulse Width - FWHM (ns)
0
5
10
15
20
25
Repetition Rate (kHz)
3000 3500 4000 4500 5000 5500
5
10
15
20
25
30
Pump Power (mW)
Output Power (mW)
Output Power (mW)
Pulse Width - FWHM (ns)
Repetiton Rate (kHz)
550
600
650
700
750
800
Pulse Width - FWHM (ns)
12
14
16
18
20
22
24
26
28
Repetition Rate (kHz)
0.55
0.6
0.65
0.7
0.75
0.8
0.85
0.9
0.95
S
p
ectral Width
(
nm
)
740 745 750 755
10
15
20
25
30
35
40
45
Wavelength (nm)
Output Power (mW)
Output
Power (mW)
Pulse Width
FWHM (ns)
Repetiton
Rate (kHz)
Spectral
Width (nm)
PHOTOPTICS 2017 - 5th International Conference on Photonics, Optics and Laser Technology
86
schematic layout). We noted that in order to
demonstrate this wavelength tunable passive Q-
switched direct diode-pumped Alexandrite laser
experimentally for the first time in the literature, we
choice to utilize this very simple cavity
configuration. However this linear cavity
configuration we used has some disadvantages
especially in the means of achieving relatively
higher output power and higher efficiency. In
particular, the use the beam coming from the BiFi
was not ideal. This caused lower output power
values to be detected in the measurements. In order
to overcome this issue, we developed an X-cavity
setup for our future studies as explained in the next
section.
Figure 8: Pulse train observed from passively Q-switched
Alexandrite at 743 nm and 750 nm with repetition rates 14
kHz and 23 kHz, respectively.
4 FUTURE STUDY
We established an astigmatically compensated 4-
mirror X-cavity direct diode-pumped Alexandrite
laser for cw experiments shown in Figure 10. The
intention of this configuration was for obtaining
higher output power from the wavelength tunable
passive Q-switched Alexandrite laser in our future
studies. It is important to have an optimized cw
cavity to obtain passive Q-switching or passive
mode-locking. As we have done previously in
Figure 1, as a preliminary to Q-switching we first
developed a stable X-cavity cw Alexandrite laser
operating in fundamental TEM
00
mode. The cavity
consisted of Brewster angle cut Alexandrite crystal,
two curved mirrors (each with a radius of curvature
of 75 mm), a highly reflecting flat back mirror (BM)
and an output coupler mirror with reflection 99.5%.
We used the same diode pump source as in Figure 1.
Moreover, as we have done previously, we kept the
crystal and pump diode temperature equal and
constant at 16
o
C using the same single water cooling
system.
Two different cavity configurations were
investigated. In the 1
st
setup, the internal cavity
dimensions are arranged as: L
1
=37.5 mm, L
2
=35
mm, L
3
=62 mm and L
4
=55 mm. The beam quality of
the laser output is measured (with ISO 11146-1
method) as
9.6
and
10.4. Since these
beam quality factors are not satisfactory, we tried to
re-optimize the X-cavity with new lengths. In this
2
nd
configuration: L
1
=53 mm, L
2
=44 mm, L
3
=135
mm and L
4
=96 mm. For this configuration, the laser
output beam had a TEM
00
beam quality and its beam
propagation factor was measured as
1.34
and
1.17
which are far better than the results
found for the 1
st
setup. The free running laser
wavelength was around ~755 nm in both cavities.
Figure 9: Annotated photograph of the wavelength-tunable passive Q-switched direct diode-pumped Alexandrite laser.
-1 0 1
x 10
-4
0
0.2
0.4
0.6
0.8
1
time (sec)
Normalized Intensity (a.u.)
743 nm pulse train, Repetition Rate=14 kHz
750 nm pulse train, Repetition Rate=23 kHz
Output
Beam
Crystal
holder
Back mirror
Intracavity
lens
λ/2 Wave plate
Pump lens
Cavity
axis
Pump Beam
SESAM
BiFi
Brewster
angle
Surface
normal
of BiFi
Wavelength Tunable Passively Q-Switched Alexandrite Laser with Direct Diode-Pumping at 635 nm
87
Figure 10: X-cavity cw Alexandrite laser setup with Brewster angle cut crystal: 5W fibre coupled red diode laser module
(1), Fibre collimator (2), λ/2 wave plate (3), Plano convex pump lens (PCX) with f=75 mm (4), curved dichroic mirror HT
at 635 nm and HR at 755 nm with radius of curvature (ROC) 75 mm (5 and 7), Brewster angle cut Alexandrite rod with
L
crystal
= 8 mm length doped with 0.22% of Cr
3+
(6), back mirror – BM (8), Output coupler OC with reflection 99.5% (9).
Figure 11 given below shows the cw output power
of the X-cavity for the two different setups.
Figure 11: Output power vs Pump power curve of cw X-
cavity Alexandrite laser at free running laser wavelength
around ~755 nm in the two cavity setups. The crystal
temperature was 16
o
C in the experiments and output
coupling was 0.5%.
As can be seen in Figure 11, the oscillation threshold
of the 2
nd
setup is much higher than the 1
st
setup. On
the other hand, as can be further seen its slope
efficiency (~30%) is higher than the slope efficiency
of the 1
st
setup and output power is increasing with
the available pump power. This suggests that the
power performance and slope efficiency of the 2
nd
setup can be further improved with more
optimization, adjustment and by utilizing more
powerful pump lasers with higher crystal
temperatures. After having completed this step, we
will plan to replace the back mirror with the SESAM
we used in Figure 2, but can now utilise and
optimise the output coupler mirror to obtain more
efficient passive Q-switched (or potentially passive
mode-locked) diode-pumped Alexandrite laser in
our future studies.
5 CONCLUSIONS
This work demonstrated experimentally for the first
time that a wavelength tunable passive Q-switched
TEM
00
operation of Alexandrite laser can be
achieved with direct red diode-pumping. The
shortest pulse generated was 550 ns (FWHM) and
the highest repetiton rate achieved was 27 kHz in
fundamental TEM
00
mode. The maximum average
output power obtained was 41 mW and 0.56 nm was
measured as the shortest spectral width. The
wavelength tuning band spanned was between 740
nm and 755 nm. The results obtained in this study
pave the way for further development, optimization
and power scaling of this new generation tunable
diode-pumped passive Q-switched (and also
potentially for passive mode-locked) Alexandrite
laser. In our future studies; higher crystal
temperature, higher pump power, higher doping
concentration, longer gain medium, optimized
(reduced) output coupler reflectivity, enhanced
cavity design (X-cavity) and careful intracavity loss
management will provide us to obtain better
performance in tunable Q-switched operation of
diode-pumped Alexandrite laser. Due to the superior
optical and thermo-mechanical properties comparing
with its counterparts, this new generation direct
diode-pumped wavelength tunable, compact, low-
cost and efficient passive Q-switched (and also
passive mode-locked) Alexandrite laser has the
potential to become an attractive source for
addressing the requirements of many near-future
crucial scientific, medical and game-changing
industrial applications such as next generation
space-borne vegetation lidar systems.
L
1
L
2
L
3
L
4
L
crystal
2
3
1
4
5
6
7
8
9
PHOTOPTICS 2017 - 5th International Conference on Photonics, Optics and Laser Technology
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ACKNOWLEDGEMENTS
We would like to acknowledge support from the
British Council and Newton Fund under Project No.
215277462. U.P. would like to acknowledge support
from TÜBİTAK (The Scientific and Technological
Research Council of Turkey) for his visit to Imperial
College London. The authors thank Dr Arkady
Major from the University of Manitoba for
providing the SESAM that was used in this study.
REFERENCES
Damzen, M.J., Thomas, G.M., Teppitaksak, A.,
Minassian, A., 2014. Progress in diode-pumped
Alexandrite lasers as a new resource for future space
lidar missions. In ICSO 2014, International
Conference on Space Optics.
Teppitaksak, A., Minassian, A., Thomas, G.M., Damzen,
M.J., 2014. High efficiency >26 W diode end-pumped
Alexandrite laser. In Vol. 22, No.13, Optics Express.
OSA.
Koechner, W., Bass, M., 2003. Solid-State Lasers:
Graduate Text, Springer-Verlag. New York.
Ghanbari, S., Akbari, R., Major, A., 2016. Femtosecond
Kerr-lens mode-locked Alexandrite laser. In Vol. 24,
No. 13, Optics Express. OSA.
Eitel, J.U.H., Vierling, L.A., Litvak, M.E., Long. D.S.,
2011. Broadband, red-edge information from satellites
improves early stress detection in a New Mexico
conifer woodland. In 115, 3640-3636, Remote Sensing
of the Environment.
Lu, T., Li, H., 2016. Atmospheric turbulence induced
synthetic aperture lidar phase error compensartion. In
381, 214-221, Optics Communications. ELSEVIER.
Pelon, J., Megie, G., Loth, C., Flamant, P., 1986.Narrow
bandwidth Q-switch alexandrite laser for atmospheric
applications. In Vol. 59, Issue 3, 213-218, Optics
Communications. ELSEVIER.
Milton, M.J.T., Gardiner, T.D., Molero, F., Galech, J.,
1997. Injection seeded optical parametric oscillator for
range-resolved DIAL measurements of atmospheric
methane. In 142, 153-160, Optics Communications.
ELSEVIER.
Teppitaksak, Thomas, G.M., Damzen, M.J., 2015.
Investigation of a versatile pulsed laser source based
on a diode seed and ultra-high gain bounce geometry
amplifiers. In Vol. 23, No. 9, Optics Express. OSA.
Ghanbari, S., Major, A., 2016. High power continuous-
wave Alexandrite laser with green pump. In 26,
075001, Laser Physics. IOP PUBLISHING.
Beyatli, E., Baali, I., Sumpf, B., Erbert, G., Leitenstorfer,
A., Sennaroglu, A., Demirbas, U., 2013. Tapered
diode-pumped continuous-wave alexandrite laser. In
Vol. 30, No. 12, J. Opt. Soc. Am. B. OSA.
Demirbas, U., Li, D., Birge, J.R., Sennaroglu, A., Petrich,
G.S., Kolodziejski, A., Kartner, F.X., Fujimoto, J.G.,
2009. Low-cost, single-mode diode-pumped
Cr:Colquiriite lasers. In Vol.17, No. 16, Optics
Express. OSA.
Sennaroglu, A., Kaertner, F.X., Fujimoto, J.G., 2007.
Low-threshold, room-temperature femtosecond
Cr
4+
:forsterite laser. In Vol. 15, No. 20, Optics
Express. OSA.
Loiko, P., Major, A., 2016. Dispersive properties of
alexandrite and beryllium hexaaluminate crystals. In
Vol. 6, No. 7, Optics Express. OSA.
Walling, J.C., Heller, D.F., Samelson, H.,Harter, D.J.,
Pete, J.A., Morris, R.C., 1985. Tunable Alexandrite
lasers: Development and Performance. In Vol. QE21,
No. 10, J. Quantum Electronics. IEEE.
Sam, C.L., Walling, J.C., Jenssen, H.P., Morris, R.C.,
O’Dell, E.W., 1980. Characteristics of alexandrite
lasers in Q-switched and tuned operations. In Vol.247,
130-136, Advances in Laser Eng and Appl. SPIE.
Wavelength Tunable Passively Q-Switched Alexandrite Laser with Direct Diode-Pumping at 635 nm
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