SUMMARY
The discussion centers on the impact of air molecule velocity on electromagnetic (EM) waves, particularly in the context of the Earth's atmosphere. It concludes that for common air molecules such as O2, N2, CO2, and H2O, their velocity does not significantly affect light absorption unless relativistic speeds are involved. The primary effects on starlight twinkling are attributed to refractive index changes due to atmospheric density variations, influenced by wind and temperature. High-frequency EM waves like gamma and X-rays experience minimal diffraction from these molecules.
PREREQUISITES
- Understanding of electromagnetic wave properties
- Knowledge of atmospheric physics, particularly refractive index
- Familiarity with gas laws and their relation to temperature and density
- Basic concepts of diffraction and absorption in optics
NEXT STEPS
- Research the effects of atmospheric refractive index on starlight visibility
- Explore the relationship between temperature, density, and wind in atmospheric physics
- Investigate the behavior of high-frequency EM waves in various media
- Learn about the principles of diffraction and how they apply to different wavelengths of light
USEFUL FOR
Astronomers, atmospheric scientists, physics students, and anyone interested in the optical effects of the atmosphere on celestial observations.