
The process of adjusting a device to ensure its outputs match known standards.Calibration is the process of adjusting a measuring instrument or experimental setup so that its readings correspond to known, traceable standards. In physics, it is the bridge between raw data and meaningful numbers: without calibration, a detector's output is just a voltage or a count, not a temperature, a mass, or a position. The concept appears across vastly different scales — from adjusting the zero point of a balance to aligning the mirrors of a gravitational-wave observatory — but the core idea is always the same: compare the device against a reference, then correct for any systematic deviation.
The term derives from the practice of comparing the bore diameter of a gun to a standard gauge ('calibre'), dating back to the 19th century. Modern scientific calibration was formalized with the establishment of international standards like the meter and kilogram in the late 1800s.
A typical calibration involves applying a known input (a standard mass, a known frequency, a reference voltage) and recording the instrument's response. The difference between the expected and observed output defines a correction function, which is then applied to all subsequent measurements. In more complex systems, like quantum computers or dark-matter detectors, calibration can be an ongoing, automated process: the device periodically measures a reference state and adjusts its parameters to compensate for drift, noise, or environmental changes.
Calibration is essential in every quantitative science and industry — from medical devices like ECG machines (as in 'Кардиограмма без розовых очков') to space telescopes mapping dark matter, where even tiny systematic errors would corrupt the results.
The 2019 redefinition of the kilogram replaced a physical metal cylinder with a fixed value of Planck's constant, meaning that mass calibration is now ultimately tied to quantum mechanics rather than a piece of metal.




