Telescopes TRIZ Cases

An apochromatic optical design combines flint glass with anomalous dispersion elements to correct chromatic aberration.

Integrating coupling portions with monoculars reduces component count and weight while enabling detachable assembly.

Retractable mirrors enable bifocal switching in a five-mirror telescope, resolving complexity trade-offs without moving primary optics.

Moving the second negative lens unit maintains adequate depth of field and stable angle of view during focusing operations.

Extending the right ascension support downwardly and backwardly reduces bending moments on the base, enabling lighter components and manual latitude adjustment.

A synthetic leather ring with fine hairs seals lens barrel gaps while providing moderate rotational resistance.

Elastic abutments in the suspension system reduce servo loads by thirty times during launch acceleration.

Parallel optical systems use field stops to reduce stray light interference and increase pixel count in viewing areas.

A camera head uses a deformable liquid lens to expand light beams for optical zooming.

Segmented baffle structure minimizes air exchange between housing zones, preventing condensation buildup on inner window surfaces during rapid thermal shifts.

A four-mirror all-reflective optical system directs light through asymmetric curved surfaces to capture multispectral images.

A four-lens group objective lens uses movable second and third groups to switch between wide-angle and high-magnification states.

A passive optical assembly channels light from dual apertures onto a single image sensor using beam splitting and relay optics.

Hard points on the monocular frame enable ambidextrous clip attachment and accessory integration, resolving pocket access bottlenecks.