SUMMARY
The sun appears red during sunrise and sunset due to Rayleigh scattering, which affects the light's wavelength as it travels through the Earth's atmosphere. At these times, the light path is longer compared to midday, causing shorter wavelengths (blue light) to scatter away, leaving predominantly red wavelengths visible. The angle of the sun's light also contributes to this phenomenon, as the incident light during these times differs significantly from that at noon.
PREREQUISITES
- Understanding of Rayleigh scattering
- Basic knowledge of light wavelengths
- Familiarity with atmospheric science
- Concept of light propagation through different mediums
NEXT STEPS
- Research Rayleigh scattering in detail
- Explore the physics of light wavelengths and their interaction with the atmosphere
- Study the effects of atmospheric particles on light perception
- Investigate the role of the sun's angle in light scattering
USEFUL FOR
Students of physics, educators in atmospheric science, photographers interested in capturing sunrise and sunset colors, and anyone curious about optical phenomena in nature.