Sekundaarikäämit
Sekundaarikäämit, literally translated as secondary lenses, are optical elements used in conjunction with primary lenses to modify or enhance the imaging system in telescopes, microscopes, cameras, and other optical instruments. These auxiliary lenses are mounted after the main objective and before the final image plane. Their purpose is to correct for aberrations, adjust magnification, change field of view, or alter focal length without needing to redesign the primary lens.
Optical functions of sekundaarikäämit include field flattening, coma correction, and astigmatism reduction. In compound microscopes, a
Secondary lenses are typically made from high‑dispersion glass or low‑index materials, depending on the aberration they
Historically, the use of secondary lenses dates back to the 18th‑century refracting telescopes, where Steinheil and
Manufacturers produce standardized secondary elements such as tube adapters, field flattener rings, and apocromic correctors. These