SUMMARY
The Candela is defined as the unit of luminous intensity in the International System of Units (SI), specifically representing the perceived brightness of light at a frequency of 540 x 1012 Hz (555 nm). It quantifies luminous intensity as 1/683 watt per steradian, incorporating human visual response to different wavelengths. The discussion highlights the Candela's reliance on perceptual factors, questioning its necessity as a base unit in SI. Additionally, it notes that while astronomers frequently use photometric units, professional astronomers primarily rely on radiometric measurements.
PREREQUISITES
- Understanding of luminous intensity and its relationship to radiant intensity.
- Familiarity with the concept of photometric units and their applications.
- Knowledge of human visual perception and its impact on light measurement.
- Basic grasp of the International System of Units (SI) and its definitions.
NEXT STEPS
- Research the NIST standards for photometric units and their definitions.
- Learn about the differences between photometric and radiometric measurements.
- Explore the human visual response functions used in photometry.
- Investigate the applications of luminous intensity in various fields, particularly astronomy.
USEFUL FOR
Students, physicists, and engineers interested in photometry, as well as astronomers and anyone involved in light measurement and perception analysis.