Análisis numérico de la prueba de la estrella

Authors

  • O. Totolhua Paleta
  • F. Renero Carrillo
  • F. Gracia Témich
  • A. Cornejo Rodríguez

Keywords:

Geometrical optics, edge, boundary effects, reflection, refraction, image forming, processing

Abstract

In this paper, we present one method of numeric analysis for the star test with MatLab (ANPEM), applied to reflecting telescope. ANPEM finds the difference between centers of the images of the annulus obtained with a Newtonian telescope and a Ritchey Chretiêne telescope with 14 and 211 cm of diameter respectively. ANPEM allows to identify quantitative the symmetry of the annulus for each reflector telescope with a central obstruction. ANPEM finds the centres of the annulus with diference between 12 to 60$\mu $m compared with the ideal numerical differences calculated with PC for the Newtonian telescope.

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Published

2003-01-01

How to Cite

[1]
O. Totolhua Paleta, F. Renero Carrillo, F. Gracia Témich, and A. Cornejo Rodríguez, “Análisis numérico de la prueba de la estrella”, Rev. Mex. Fís., vol. 49, no. 6, pp. 549–0, Jan. 2003.

Issue

Vol. 49 No. 6 (2003): Revista Mexicana de Física.

Section

Articles

License

Authors retain copyright and grant the Revista Mexicana de Física right of first publication with the work simultaneously licensed under a CC BY-NC-ND 4.0 that allows others to share the work with an acknowledgement of the work's authorship and initial publication in this journal.