What are the two main natural sources of background radiation?
Terrestrial radiation (U, Th, K in rocks/soils) and cosmic radiation (muons/neutrons from space).
Typical global natural background dose?
~2.4 mSv/yr (UNSCEAR).
Typical terrestrial dose?
1–2 mSv/yr, up to 5+ mSv/yr in granites.
Why do terrestrial radiation levels vary?
Rock type, soil gas permeability, radon levels, building materials.
What radionuclides dominate terrestrial background?
U-238, Th-232, K-40.
What is radon and why is it important?
Radioactive gas from U-decay; main source of natural dose; varies strongly by geology.
Typical radon contribution to dose?
1 mSv/yr average; >10 mSv/yr in hotspots.
Why does cosmic radiation vary with altitude?
Thinner atmosphere → less shielding → higher particle flux.
Cosmic radiation at sea level?
0.3 mSv/yr.
Cosmic radiation during a long-haul flight?
2–5 µSv/hr.
Why is cosmic dose higher at the poles?
Weaker geomagnetic shielding → more cosmic rays reach atmosphere.
Legal public annual dose limit from nuclear activities?
1 mSv/yr (ICRP).
Typical design target for repository during operation?
<0.3 mSv/yr.
Long-term post-closure dose target?
0.01–0.1 mSv/yr.
Expected real repository flux?
Often <0.001 mSv/yr.
How does natural dose compare to regulated nuclear releases?
Natural variability is 100–1000× higher than regulated doses.
Chernobyl total release?
~5.2 EBq.
Chernobyl radiation in 1986 hotspots?
>1000 µSv/hr.
Chernobyl radiation today?
0.2–5 µSv/hr.
Fukushima total release?
~940 PBq.
Fukushima 2011 off-site dose rate?
20–300 µSv/hr.
Fukushima decontaminated area dose today?
0.2–1 µSv/hr.
Global weapons testing fallout dose in 1960s?
+0.1–0.2 mSv/yr.
Global fallout dose today?
<0.01 mSv/yr.