KONUS

Konus refers to a family of gamma-ray detectors used in space astronomy, best known for the KONUS-Wind instrument. The KONUS detectors are designed to monitor the sky for high-energy events such as gamma-ray bursts and solar flares, providing spectral and temporal information to complement observations from other spacecraft.

The KONUS instrument on Wind consists of two nearly identical scintillation detectors that view the sky from different directions, giving a broad field of view. They measure gamma rays over a wide energy range and deliver data products such as light curves, spectra, and burst-related timing information. This enables rapid detection of transient events and detailed follow-up analysis in coordination with other missions and ground-based facilities.

KONUS-Wind has operated since its launch in 1994 and has contributed to long-term studies of gamma-ray bursts, improving the ability to characterize their spectral evolution and temporal structure. The instrument has also provided valuable data during solar activity and served as a cross-calibration reference for other gamma-ray detectors.

Beyond KONUS-Wind, the name appears in various contexts within space science and astronomy and may be found as a surname in some languages. The primary scientific association remains the gamma-ray detector technology used to study high-energy transient phenomena.