Ratio of cosmic and cosmogenic radiation

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SUMMARY

The discussion centers on the ratio of cosmogenic radiation to cosmic radiation at sea level, highlighting that cosmic radiation is estimated at approximately 300 microsieverts per year. It is established that muons constitute over half of this radiation, with the remainder comprising electrons, positrons, and photons from cascade events. The conversation emphasizes the need to analyze cosmic radiation attenuation and the induced activity in various mediums, including air, water, and minerals, to derive accurate ratios.

PREREQUISITES
  • Understanding of cosmic radiation and its components, specifically muons and cascade events.
  • Knowledge of isotopes related to cosmic radiation, including T, Be-7, Be-10, and C-14.
  • Familiarity with radiation measurement units, particularly microsieverts.
  • Basic principles of nuclear reactions and cosmogenic production.
NEXT STEPS
  • Research cosmic radiation attenuation and its effects on different materials.
  • Study the production and decay of isotopes created by cosmic radiation.
  • Explore the role of muons in cosmic radiation and their interactions with matter.
  • Investigate methodologies for measuring cosmogenic radiation in various environments.
USEFUL FOR

Researchers in astrophysics, environmental scientists, and anyone studying the effects of cosmic radiation on Earth’s atmosphere and surface materials.

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Air stops most cosmic radiation.
Yet some particles do reach sea level.
The cosmic radiation at sea level is estimated at around 300 microsieverts per year.
Cosmic radiation also causes nuclear reactions in air that stops it.
Many isotopes created by cosmic radiation are stable, or short lived and remain in air.
Heaviest common nucleus in air is O-16. Of nuclei lighter than 16, only 4 are radioactive but have half-life over 21 minutes. These are T (12 years), Be-7 (53 days), Be-10 (1,5 million years) and C-14 (5700 years).
What is the ratio of cosmogenic radiation to cosmic radiation on sea level?
 
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snorkack said:
What is the ratio of cosmogenic radiation to cosmic radiation on sea level?
It's an interesting question. I'm trying to find a good answer. One has to look at the attenuation of cosmic radiation, and types, and then look at the induced-activity in the air and at the surface - water vs plant vs mineral.

Muons make up more than half of the cosmic radiation at sea level, the remainder being mostly electrons, positrons and photons from cascade events. (Richtmyer)
http://hyperphysics.phy-astr.gsu.edu/hbase/astro/cosmic.html#c2

See Figure 24.3 http://pdg.lbl.gov/2011/reviews/rpp2011-rev-cosmic-rays.pdf

Some information on cosmogenic production here - http://www.whoi.edu/fileserver.do?id=133844&pt=2&p=146949
 

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