SUMMARY
The intensity of cosmic rays is highest at approximately 20 km above Earth's surface, where secondary muons are generated from collisions between primary cosmic rays and atmospheric atoms. Experimental studies confirm that as altitude increases beyond this point, the intensity of cosmic rays decreases due to a lower concentration of atmospheric atoms, resulting in fewer collisions and thus fewer muons. Primary cosmic rays originate from space, and their detection on Earth primarily involves secondary cosmic rays produced in the atmosphere. This phenomenon highlights the relationship between altitude and cosmic ray intensity, contradicting any claims that cosmic rays originate more from Earth.
PREREQUISITES
- Understanding of cosmic ray physics
- Knowledge of atmospheric composition and behavior
- Familiarity with particle interactions in high-energy physics
- Basic principles of ionization and radiation detection
NEXT STEPS
- Research the mechanisms of cosmic ray production and detection
- Study the effects of altitude on particle collision rates
- Explore the role of muons in cosmic ray experiments
- Investigate the atmospheric conditions affecting cosmic ray intensity
USEFUL FOR
Astronomers, physicists, atmospheric scientists, and anyone interested in the origins and behavior of cosmic rays in relation to Earth's atmosphere.