Quetelet rings are a type of optical interference pattern occurring at an illuminated reflective surface covered by fine particles, such as a dusty mirror. It is named after the astronomer Adolphe Quetelet, who observed the phenomenon and explained its formation. A slight variation of the setup is sometimes referred to as Newton's dusty mirror experiment, since Isaac Newton had already discovered the phenomenon by the end of 17th century, but did not interpret or explain it.[1]
Quetelet rings on a dusty mirror
Quetelet rings arise from interference of the light that is first scattered by a particle and then reflected by the surface, with the light that first gets reflected and then scattered by the particle. Contributions of these two paths to the scattering differ by a phase factor that depends on the wavelength and the angles of light incidence and scattering. Depending on the phase difference, these contributions may interfere constructively (contributing to a bright band) or destructively (contributing to a black band). In the case of illumination by white light the patterns produced by different wavelengths are slightly misaligned with each other and that results in a coloring of the rings. The pattern is most noticeable around the reflection image of the light source. The closer the images of the light source and the observer are on the mirror and the closer the particles are to the reflective surface, the broader are the interference fringes.
Galleryedit
Photographs of Quetelet rings on a mirror covered with talcum powder. The camera and the light source are placed in five meters from the mirror; the distance between the camera and the light source increases up to 50 cm. The camera is focused at infinity.
Light source right next to the objective of the camera
Light source at 10 cm from the objective of the camera
Light source at 25 cm from the objective of the camera
Light source at 50 cm from the objective of the camera
A video demonstrating Quetelet rings as seen on a mirror covered in flour while the flashlight moves around the observer.
Wilfried Suhr and Joachim Schlichting: Coloured rings produced on transparent plates (PDF; 990 kB), Institut für Didaktik der Physik - Universität Münster
Dietrich Zawischa: Quetelet rings, Institut für Theoretische Physik, Universität Hannover
January 01, 1970
quetelet, rings, this, article, require, copy, editing, grammar, style, cohesion, tone, spelling, assist, editing, april, 2024, learn, when, remove, this, message, type, optical, interference, pattern, occurring, illuminated, reflective, surface, covered, fine. This article may require copy editing for grammar style cohesion tone or spelling You can assist by editing it April 2024 Learn how and when to remove this message Quetelet rings are a type of optical interference pattern occurring at an illuminated reflective surface covered by fine particles such as a dusty mirror It is named after the astronomer Adolphe Quetelet who observed the phenomenon and explained its formation A slight variation of the setup is sometimes referred to as Newton s dusty mirror experiment since Isaac Newton had already discovered the phenomenon by the end of 17th century but did not interpret or explain it 1 Quetelet rings on a dusty mirror Quetelet rings arise from interference of the light that is first scattered by a particle and then reflected by the surface with the light that first gets reflected and then scattered by the particle Contributions of these two paths to the scattering differ by a phase factor that depends on the wavelength and the angles of light incidence and scattering Depending on the phase difference these contributions may interfere constructively contributing to a bright band or destructively contributing to a black band In the case of illumination by white light the patterns produced by different wavelengths are slightly misaligned with each other and that results in a coloring of the rings The pattern is most noticeable around the reflection image of the light source The closer the images of the light source and the observer are on the mirror and the closer the particles are to the reflective surface the broader are the interference fringes Gallery editPhotographs of Quetelet rings on a mirror covered with talcum powder The camera and the light source are placed in five meters from the mirror the distance between the camera and the light source increases up to 50 cm The camera is focused at infinity nbsp Light source right next to the objective of the camera nbsp Light source at 10 cm from the objective of the camera nbsp Light source at 25 cm from the objective of the camera nbsp Light source at 50 cm from the objective of the camera A video demonstrating Quetelet rings as seen on a mirror covered in flour while the flashlight moves around the observer source source source source source Quetelet rings in motionReferences edit Karl Exner Ueber die Newtonschen StaubringeExternal links editWilfried Suhr and Joachim Schlichting Coloured rings produced on transparent plates PDF 990 kB Institut fur Didaktik der Physik Universitat Munster Dietrich Zawischa Quetelet rings Institut fur Theoretische Physik Universitat Hannover Retrieved from https en wikipedia org w index php title Quetelet rings amp oldid 1221426468, wikipedia, wiki, book, books, library,
