2012
DOI: 10.1364/josab.29.001270
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Modeling of amplified spontaneous emission, heat deposition, and energy extraction in cryogenically cooled multislab Yb^3+:YAG laser amplifier for the HiLASE Project

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Cited by 49 publications
(30 citation statements)
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“…The important parameters to be estimated are: maximum required DM deformation (stroke), spatial frequency and temporal evolution of the aberrations. The aberrations can be calculated with simulations [3][4][5] using numerical models or estimated by previous experiments on similar systems [6,7] .…”
Section: Design Parametersmentioning
confidence: 99%
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“…The important parameters to be estimated are: maximum required DM deformation (stroke), spatial frequency and temporal evolution of the aberrations. The aberrations can be calculated with simulations [3][4][5] using numerical models or estimated by previous experiments on similar systems [6,7] .…”
Section: Design Parametersmentioning
confidence: 99%
“…For example, in the case of the HiLASE laser [8] four numerical models have been developed in order to estimate the thermal effects within the gain media, optical aberrations introduced by the main multi-slab amplifier (see Figure 1) and the wavefront correction. The first model simulates the effect of amplified spontaneous emission (ASE) in the 1 2 S. Bonora et al gain media [7] ; the second computes the temperature distribution, thermal stresses and estimates the induced optical aberrations [3] (see Figure 1(b) for sample result).…”
Section: Thermo-optical Simulationsmentioning
confidence: 99%
“…The energetics modeling of the amplifiers is provided by our in-house-developed numerical code [20]. The code works in discrete time steps.…”
Section: Numerical Modelling Of Laser Amplifiersmentioning
confidence: 99%
“…First, the amplifier head was studied and crucial parameters were estimated by two numerical models, including the aberration induced by thermal loading of the gain media [20,21]. In order to estimate the aberration of the output laser beam, another main source of aberrations was estimated by a different numerical model.…”
Section: Wavefront Correction By a Deformable Mirrormentioning
confidence: 99%
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