finesse.thermal.hello_vinet
Hello-Vinet equations for thermal lenses in cylindrical mirrors. Higher order mode thermal effects are not implemented here. Therefore all the functions return some axially symmetric data.
Equations all based on [32]:
Jean-Yves Vinet, “On Special Optical Modes and Thermal Issues in Advanced Gravitational Wave Interferometric Detectors” Living Review 2009
Functions
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Evaluates a Fourier-Bessel decomposition fit performed with   | 
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Returns beam intensity overlap coefficients as calculated by Eq 3.33 in [32].  | 
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Performs a Fourier-Bessel decomposition of some axisymmetric irradiance distribution.  | 
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Calculates the intesity of incident on a mirror surface from an ideally thin ring radiator.  | 
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Computes the 2D substrate temperature distribution per Watt of absorbed power in each of the coating and substrate for an arbitrary axisymmetric heating irradiance computed with   | 
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Computes the 2D substrate temperature distribution per Watt of absorbed power in each of the coating and substrate from a HG00 beam.  | 
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Computes the depth displacements throughout the bulk of an optic due to coating absorption.  | 
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Computes the depth displacements throughout the bulk of an optic due to coating absorption.  | 
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Computes the depth displacement change of the surface of an optic due to coating absorption.  | 
Computes the depth displacement change of the surface of an optic due to coating absorption.  | 
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Computes the depth displacement change of the surface of an optic due to bulk absorption from a generic axisymmetric heating profile.  | 
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Computes the depth displacement change of the surface of an optic due to bulk absorption from a HG00 beam.  | 
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Computes the substrate thermal lens per Watt of absorbed power in each of the coating and substrate for an arbitrary axisymmetric heating irradiance computed with   | 
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Computes the substrate thermal lens per Watt of absorbed power in each of the coating and substrate from a HG00 beam.  | 
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Compute the roots of the equation  |