The sine, a fundamental trigonometric function, is defined as the ratio of the length of the side opposite an acute angle in a right triangle to the hypotenuse's length. This concept, extended beyond right triangles, underpins periodic phenomena in mathematics and physics. Authors such as Thomas Hobbes explored sine in the context of refraction, noting its proportional relationship to medium densities, while Isaac Newton applied it to optical refraction and wave propagation.
Henry Coddington emphasized its role in geometric optics, linking angles of incidence and refraction through sine ratios. These varied approaches underscore sine’s dual role as a mathematical tool and a descriptive element in natural laws, bridging geometry, physics, and engineering.