Hoghton's camera and telescope
Résumé
The third-order aberration formulae we have proved in a previous paper, starting from Fermat's principle and from the idea of stigmatic paths, are here applied to analyze and to project Houghton's cameras and Houghton-Cassegrain's telescopes. The final values of the radii of the two-lens corrector are obtained taking into account also the thickness of lenses and the fifth-order aberrations.
Domaines
Physique mathématique [math-ph]
Origine : Fichiers produits par l'(les) auteur(s)
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