<?xml version="1.0" encoding="ISO-8859-1"?><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance">
<front>
<journal-meta>
<journal-id>1562-3823</journal-id>
<journal-title><![CDATA[Revista Boliviana de Física]]></journal-title>
<abbrev-journal-title><![CDATA[Revista Boliviana de Física]]></abbrev-journal-title>
<issn>1562-3823</issn>
<publisher>
<publisher-name><![CDATA[Sociedad Boliviana de Física]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S1562-38232012000400013</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Optical study of the laser beam propagation on Nd:YAG crystal slab for space LIDAR missions]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Gazeas]]></surname>
<given-names><![CDATA[Kosmas]]></given-names>
</name>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Tzeremes]]></surname>
<given-names><![CDATA[George]]></given-names>
</name>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Armandillo]]></surname>
<given-names><![CDATA[Errico]]></given-names>
</name>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,ESTEC European Space Agency ]]></institution>
<addr-line><![CDATA[ ]]></addr-line>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>00</month>
<year>2012</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>00</month>
<year>2012</year>
</pub-date>
<volume>20</volume>
<numero>20</numero>
<fpage>36</fpage>
<lpage>38</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.bo/scielo.php?script=sci_arttext&amp;pid=S1562-38232012000400013&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.bo/scielo.php?script=sci_abstract&amp;pid=S1562-38232012000400013&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.bo/scielo.php?script=sci_pdf&amp;pid=S1562-38232012000400013&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[The present paper reports on the development of a simulation and modeling tool which allows to estimate the propagation effects on a laser beam passing through a laser-diode-pumped Nd:YAG slab amplifier. This in-house research work is motivated by current ESA spaceborne LIDAR programs (ADM, Earth Care) as a mean to provide understanding of the LIDAR beam pointing stability as results of thermal and mechanical stresses. A dynamic model has been generated that can simulate the optical characteristics of the laser beam propagation, as a result of the various thermal and mechanical processes occurring inside the laser Pumping Unit and the thermal lensing occurring along the crystal slab. The simulation results and their comparison with actual laboratory tests are being presented and discussed. The model developed is based on the Finite Element Model (FEM) methodology, where the slab as an active element is "broken" down into interdependent segments, each simulated as being heated by an individual LD source. The light beam is propagated along the slab using dynamically varying boundary conditions, to the next so to account for the cumulated thermal and mechanical loads.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Nd:YAG laser]]></kwd>
<kwd lng="en"><![CDATA[thermal lensing]]></kwd>
<kwd lng="en"><![CDATA[LIDARS]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <p align="center"><font size="4" face="Verdana"><strong>Optical study of the laser beam propagation on Nd:YAG   crystal slab for space LIDAR missions</strong></font></p>     <p align="center">&nbsp;</p>     <p align="center"><strong><font size="3" face="Verdana">Kosmas   Gazeas, George Tzeremes and Errico Armandillo</font></strong></p>     <p align="center"><strong><font size="2" face="Verdana">European   Space Agency, ESTEC, Mechatronics and Optics Division Keplerlaan 1, 2200AG,   Noordwijk, The Netherlands</font></strong></p>     <p align="center"><strong><font size="2" face="Verdana">Tel:   +31 71 5656743, Fax: +31 71 5655430,</font></strong></p>     <p align="center"><strong><font size="2" face="Verdana"> E-mail: Kosmas.Gazeas@esa.int,   kgaze@physics.auth.gr</font></strong><font size="2" face="Verdana"></font></p> <hr>     <p><font size="2" face="Verdana"><b>SUMMARY</b></font></p>     <p><font size="2" face="Verdana">The present paper reports on the   development of a simulation and modeling tool which allows to estimate the   propagation effects on a laser beam passing through a laser-diode-pumped Nd:YAG   slab amplifier. This in-house research work is motivated by current ESA   spaceborne LIDAR programs (ADM, Earth Care) as a mean to provide understanding   of the LIDAR beam pointing stability as results of thermal and mechanical   stresses. A dynamic model has been generated that can simulate the optical   characteristics of the laser beam propagation, as a result of the various   thermal and mechanical processes occurring inside the laser Pumping Unit and   the thermal lensing occurring along the crystal slab. The simulation results   and their comparison with actual laboratory tests are being presented and   discussed. The model developed is based on the Finite Element Model (FEM)   methodology, where the slab as an active element is &quot;broken&quot; down   into interdependent segments, each simulated as being heated by an individual   LD source. The light beam is propagated along the slab using dynamically   varying boundary conditions, to the next so to account for the cumulated   thermal and mechanical loads.</font></p>     <p><font size="2" face="Verdana"><b>Key words: </b>Nd:YAG laser, thermal lensing, LIDARS</font></p><hr>     <p><font size="2" face="Verdana"><b>INTRODUCTION</b></font></p>     ]]></body>
<body><![CDATA[<p><font size="2" face="Verdana">LIDARs in space require reliable   operation of high power laser transmitters. It is the case for ESA ADM and   EarthCare missions where high power UV lasers are being used in an   oscillator-multipass amplifier configuration to reach the required energy level   and characteristics (Figure 1). ESA space LIDAR programs use both high power   Nd:YAG slab, with diode-laser (LD) pumped. In these configurations,   thermo-mechanical behavior of the slab can affect seriously the output laser   beam characteristics, specifically the most critical variables which can play   an important role in the output laser beam are the:</font></p>     <p><font size="2" face="Verdana">•Coldplate temperature (TCP)</font></p>     <p><font size="2" face="Verdana">•Laser Diode physical   characteristics and location</font></p>     <p><font size="2" face="Verdana">•Slab geometry</font></p>     <p><font size="2" face="Verdana">•Input beam characteristics</font></p>     <p><font size="2" face="Verdana">•Collimating optics</font></p>     <p><font size="2" face="Verdana">•Operating conditions (air/vacuum,   ambient temp.)</font></p>     <p><font size="2" face="Verdana">To model such processes, it is to be   noted that since the number of variables is too large to allow a closed form   solution for the thermal lensing of the crystal slab, Finite Element Method   (FEM) is proposed and used to compute the combined thermal, mechanical and   optical effects.</font></p>     <p><font size="2" face="Verdana"><b>MOTIVATION OF THIS WORK</b></font></p>     <p><font size="2" face="Verdana">energy loss at minimum. Also we will   have the ability to predict the outgoing laser beam profile and divergence.   This will give direct information for the actual lenses need to be applied   before and after the PU, in order to focus the beam and preserve its shape and   energy density.</font></p>     ]]></body>
<body><![CDATA[<p><font size="2" face="Verdana"><img width=343 height=73 id="Imagen 1" src="/img/revistas/rbf/v20n20/v20n20a13-image001.png"></font></p>     <p><font size="2" face="Verdana">Figure 1. A schematic of the amplifier PU.</font></p>     <p><font size="2" face="Verdana">Nd:YAG   CRYSTAL SLAB GEOMETRY</font></p>     <p><font size="2" face="Verdana">The crystal slab geometry is shown   in Figure 2. A laser beam with a Gaussian profile at 1064 nm enters the crystal   parallel along the long axis and bounces 5 times on the top and 5 on the bottom   inner surfaces. The other two side surfaces are attached to the cold plates,   pumping out the accumulated heat. Boundary conditions are controlled by heat   drain from the two cold plates and the energy emitted from the 8 pumping laser   diodes at 808 nm.</font></p>     <p><font size="2" face="Verdana"><b>THERMAL LENSING</b></font></p>     <p><font size="2" face="Verdana">The final goal is to achieve fully   controlled boundary conditions and direct view of the outgoing laser beam. This   way we can predict the necessary modifications needed to preserve the laser   energy and amplification efficiency reducing conditions. Each cross section is   converted to a “refractive index matrix”, acting as lens for the laser beam.   The number of thermal lenses is a variable parameter in the performance model   for fine tuning and resolution control. Laser beam</font></p>     <p><font size="2" face="Verdana">“interacts” with “thermal lenses”,   as a normal lens. We assume ray optics (geometrical/linear optics) for the beam   propagation and no scatter through diffraction through OPD. Refraction is taken   into account via the beam’s angle of incidence on the thermal lenses (Snell   law).</font></p>     <p><font size="2" face="Verdana"><img width=363 height=81 id="Imagen 2" src="/img/revistas/rbf/v20n20/v20n20a13-image002.png"></font></p>     <p><font size="2" face="Verdana"><b>Figure 2. The 1064 nm laser beam   is travelling along the Nd:YAG slab, bouncing 10 times on the inner slab   surface, while the laser diodes are pumping energy from top and bottom,   producing 8 hot spots on the crystal slab. The laser beam enters the crystal   from left, exits from the right and its turned backwards with a mirror, causing   the beam to enter the slab again, following the same path.</b></font></p>     <p><font size="2" face="Verdana"><b>THE DEVELOPED SIMULATION GUI</b></font></p>     ]]></body>
<body><![CDATA[<p><font size="2" face="Verdana">Our simulations resulted in a   graphical user interface (GUI) control panel, where the user can insert all   variables necessary for the crystal slab geometry and boundary conditions (TCP   and LD boundary temperatures, slab geometry, number of LDs, slab’s refractive   index, etc), as shown in Figure 3. The incoming beam is assumed to have a   Gaussian profile (could be an input variable in a forthcoming version) with a   user- defined divergence and the outgoing beam is given for both single and   double laser beam pass through the crystal slab. Beam can be shifted   up-down-left-right in order to examine the effect of poor optical alignment.</font></p>     <p><font size="2" face="Verdana"><b>MECHANICAL DEFORMATION – STRESS</b></font></p>     <p><font size="2" face="Verdana">Deformation through expansion is   taken into account in calculations. This effect does not have any significant   direct optical effect. Indirectly, however, it affects conductivity of the   crystal slab with the CP, changing boundary conditions. Expansion leads to   stress of slab and conductivity variability. This in turn leads in new thermal   profile, which can be input as step 1 in our study. Variations of the initial   parameters (geometry and environmental effects) as well as the boundary   conditions result in a laser beam deformation pattern, according to the input   parameters. An example is given in Figure 4.</font></p>     <p><font size="2" face="Verdana"><b>SIMULATIONS – EXPERIMENTAL TESTS</b></font></p>     <p><font size="2" face="Verdana">It is observed that the boundary   temperature variations affect drastically the outgoing laser beam shape,   resulting in an unfocused and highly divergent non-Gaussian beam. Recent   experimental tests demonstrated that small environmental temperature changes as   small as 1° C can drastically affect the performance of the PU. This is a   result of multiple physical factors being affected simultaneously from   temperature (such as the LD’s wavelength of operation, the LD’s optical to   optical efficiency, the absorption profile of the Nd:YAG crystal, the crystal   boundary temp. conditions, ASE etc.). Our simulations can resample the existing   experimental results and can predict the laser beam profile as a function of   the boundary conditions, giving accurate quality results (Figure 5). Moreover,   additional results have to be collected for the algorithm calibration. This   will be done by in-situ experimental tests performed on a Nd:YAG crystal slab   and its amplification performance as a function of temperature perturbations.   These final results will provide the actual images required for accurate   calibration of our algorithms.</font></p>     <p><font size="2" face="Verdana"><img width=327 height=138 id="Imagen 3" src="/img/revistas/rbf/v20n20/v20n20a13-image003.png"></font></p>     <p><font size="2" face="Verdana"><b>Figure 3. The developed GUI can   simulate the thermal profile inside the crystal slab and predict the outgoing   laser beam deformation after a single and double pass through the slab. All   boundary conditions can be controlled (LD temp., CP temp., laser beam offset,   ambient temp., input laser beam profile (assumed Gaussian here), crystal   geometry etc).</b></font></p>     <p><font size="2" face="Verdana"><img width=339 height=136 id="Imagen 4" src="/img/revistas/rbf/v20n20/v20n20a13-image004.png"></font></p>     <p><font size="2" face="Verdana"><b>Figure 4. Small asymmetries of   the boundary conditions result in a asymmetric laser beam deformation, visible   in both single and double pass through the slab (panels on the right). Note   that even 0.5° C difference between the TCP and 1° C between the LD heating   cause a significant asymmetry on the outgoing laser beam at the bottom-right   panel.</b></font></p>     <p><font size="2" face="Verdana"><img width=347 height=227 id="Imagen 5" src="/img/revistas/rbf/v20n20/v20n20a13-image005.png"></font></p>     ]]></body>
<body><![CDATA[<p><font size="2" face="Verdana"><b>Figure 5. A comparison of actual   experimental tests, provided by Selex Galileo (left two panels) with our   simulations (right two panels). The results are significantly similar. Precise   model calibration and fine tuning of the parameters will allow us to predict   the shape of the outgoing beam from the amplifier PU.</b></font></p>     <p><font size="2" face="Verdana"><b>CONCLUSIONS</b></font></p>     <p><font size="2" face="Verdana">Experimental tests are currently   undertaken at ESA/ESTEC establishment, in order to validate the thermal lensing   performance model and calibrate/quantify/validate the thermal lensing effect.   However, tests already performed by Selex Galileo in Italy show that CP   temperature mainly drives the laser beam divergence and focusing ability (shape   and profile), while temperature uniformity is the key answer to laser   amplification optimization (as well as minimization of the laser beam dimensions).   Our results are successful and the developed performance model is a promising   tool for studying the thermal lensing effect, caused by a given thermal profile   along the Nd:YAG slab.</font></p>      ]]></body>
</article>
