SUMMARY
The discussion focuses on the impact of distance on the blue/red irradiance ratio in Rayleigh scattering. It is established that when the sun is overhead, light travels through approximately 10-20 miles of atmosphere, allowing over 90% of light to reach the observer, resulting in a predominantly blue appearance. Conversely, during sunset, light travels through about 100 miles of atmosphere, scattering blue light more significantly and causing the sun to appear red or orange. The wavelength of blue light is approximately half that of red light, contributing to this phenomenon.
PREREQUISITES
- Understanding of Rayleigh scattering principles
- Knowledge of light wavelengths (specifically blue and red)
- Basic atmospheric science concepts
- Familiarity with the geometry of the Earth and atmospheric thickness
NEXT STEPS
- Research the mathematical models of Rayleigh scattering
- Explore the effects of atmospheric composition on light scattering
- Study the relationship between light wavelength and scattering intensity
- Investigate the impact of altitude on atmospheric light scattering
USEFUL FOR
Students and professionals in atmospheric science, physicists studying light behavior, and educators teaching concepts of optics and environmental science.