next previous
Up: Development of a

2. Active optics and large deformations

To generate a peculiar flexure the elasticity problem is to determine the variable thickness distribution associated with a given loading configuration or the reverse, i.e. the loading configuration associated with a constant thickness, solving the elastical equilibrium equations, with the associated boundary conditions (simply supported or clamped edges). In the case of small deformations applied to a circular plate, this process is generally reduced to solve a differential equation between the flexure, the thickness distribution and the loading configuration, one of these last two functions being unknown. But when the flexure become larger, the forces and moments applied to an element generate radial and tangential stress tex2html_wrap_inline1037 and strains tex2html_wrap_inline1039 in the mirror structure (see Fig. 3 (click here)). Taking into account these forces we have to solve a differential system with three 3tex2html_wrap_inline1041 order, non-linear, coupled and non-homogeneous equations.

  figure251
Figure 3: Forces and moments for an element of the deformed mirror

We consider the quadratic deformation W(r)=W0(1-r2/a2), where W0 is the maximal deformation needed for the variable curvature mirror and a the radius at the edge of the mirror. Using a circular plate with a variable thickness distribution t(r) under an uniform load q, the differential system of equilibrium equations can be written as follow:
eqnarray259
where M(r,t) are the bending moments and N(r,t) the tensiles forces associated (Ferrari 1993).

Using the expression of the radial and tangential stress tex2html_wrap_inline1037 and strains tex2html_wrap_inline1039 given by Timoshenko & Woinowsky-Krieger and those of M(r,t) and tex2html_wrap_inline1039, functions of the flexion W(r) and the thickness t(r), this system can be transformed into another one in which the relation between W(r) and t(r) is underlined.
eqnarray283
where the radial shearing force, for an uniform loading configuration, is equal to tex2html_wrap_inline1073.

Behind this point we used a numerical method, integrating the equations, in order to determine the solutions of the differential system. But unlike usual elasticity codes which calculate the deformations of a given structure, we answer the problem backwards. We determine a structural parameter of the mirror, its thickness distribution t(r), from the desired flexure W(r). This new method is well adapted to the problem and permits to obtain solutions fast, avoiding numerous iterations between the inputed structure and the resulting deformation (Ferrari 1993).

The numerical code gives us the thickness distribution, the bending moments, the tensile forces and the total stress to insure that we stay in the elasticity domain of the material. From these results we first can fix the limit of validity of the small deformations approximation. Up to a flexion amplitude equal to 1/3 of the mirror's mean thickness (i.e. a flexion ratio tex2html_wrap_inline1079) both theories give the same thickness distributions with only 2 or 3% deviations. After this limit, the non-linear effects introduced by the shearing forces into the mirror become important and the differences between the solutions can reach 50% for a flexion ratio equal to 1.5 (LOOM 1991).

The code calculates also the value of the load q to apply in order to achieve the desired radius of curvature (or the flexion ratio tex2html_wrap_inline1083). This relation is displayed in Fig. 4 (click here) in a dimensionless form for stainless steel. This material having a Poisson ratio tex2html_wrap_inline1085 equal to 0.315, against 0.20 for a glass, the bending moments and thus the flexion achieved are larger, but the stress are also higher. The limit of the small deflections approximation is evident in this figure where the curves obtained with the two different theories diverge for flexion ratios above 1/3.

  figure351
Figure 4: Load/Flexion relations in the case of a simply supported plate given by the small and large deformations theories


next previous
Up: Development of a

Copyright by the European Southern Observatory (ESO)