Double light source Ronchi Tester for detection of ruling rotations

dc.contributor.authorJuan Núñez
dc.contributor.authorJavier Salinas-Luna
dc.contributor.authorYuliette Katinka Nuñez-Moreno
dc.contributor.authorJ. H. Castro-Chacón
dc.contributor.authorJosé Luis Monay-Arredondo
dc.contributor.authorBenjamín Martínez-Chávez
dc.contributor.authorGustavo Enrique Ramos-Alcaraz
dc.contributor.authorMarlen Meza‐Sánchez
dc.contributor.authorMiguel Alonso
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T15:36:45Z
dc.date.available2026-03-22T15:36:45Z
dc.date.issued2024
dc.descriptionCitaciones: 1
dc.description.abstractAbstract In this work, a modified Ronchi tester with a double light source has been implemented for evaluating and minimizing the rotation angle of the Ronchi ruling. The ruling rotations produced by positioning errors can become very small and could be going unnoticed (0.1°), however we have demonstrated that for these angle sizes the aberrations in the wavefront can not be completely neglicted. Accordingly with a rotatory mechanical device for correctioning the Ronchi ruling has been also added with this proposals. With our aim, in spite of non-straight shape that the ronchigrams can present in the patterns, the process of the ruling rotation degree measuring has hurled some experimental results when three concave mirrors: a concave spherical mirror, a concave parabolic mirror (the primary mirror of a Newtonian telescope) and a spherical concave mirror (the primary mirror of a Maksutov-Cassegrain telescope) have been tested.
dc.identifier.doi10.1088/1402-4896/ad368d
dc.identifier.urihttps://doi.org/10.1088/1402-4896/ad368d
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/53382
dc.language.isoen
dc.publisherIOP Publishing
dc.relation.ispartofPhysica Scripta
dc.sourceEnsenada Institute of Technology
dc.subjectLight source
dc.subjectOptics
dc.subjectRotation (mathematics)
dc.subjectComputer science
dc.titleDouble light source Ronchi Tester for detection of ruling rotations
dc.typearticle

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