SUMMARY
The discussion focuses on the detectable wavelengths of electromagnetic energy at the Earth's surface, specifically in the infrared spectrum. Approximately 50% of the light reaching the surface is infrared, despite expectations that longer wavelengths would be more absorbed by the atmosphere. Atmospheric moisture significantly absorbs infrared radiation, which is why infrared telescopes, such as those on Mauna Kea, are positioned at high altitudes to minimize this interference. Additional resources, including diagrams and detailed explanations of solar radiation levels, are provided for further understanding.
PREREQUISITES
- Understanding of electromagnetic spectrum terminology
- Familiarity with infrared radiation properties
- Knowledge of atmospheric absorption effects
- Basic concepts of telescope positioning and environmental factors
NEXT STEPS
- Research the specific wavelengths of infrared light detectable on Earth
- Explore atmospheric absorption characteristics of different wavelengths
- Learn about the design and location considerations for infrared telescopes
- Investigate solar radiation levels at various altitudes and their implications
USEFUL FOR
Researchers in atmospheric science, astronomers utilizing infrared telescopes, and environmental scientists studying solar radiation effects on Earth.