RPR-13
Skyshine snapshot
Ḣ = k Ḣ0 B Ω / d². Roof scatter raining down outside the vault.
Governing equation
where
- \dot H_0
- Isocentre rate toward roof (mSv/h)
- B
- Roof transmission (—)
- \Omega
- Roof solid angle (sr)
- d
- Horizontal distance (m)
- k
- Skyshine constant k (m²)
- \dot H
- Skyshine dose rate (µSv/h)
Lecture brief
Historical brief
Inverse-square, half-value layer, ICRP weighting and ALARA are the protection craft since the 1920s commissions. The lab computes transmission, equivalent dose and a shielding snapshot. This sheet (RPR-13 — Skyshine snapshot) is the form associated with NCRP 151 skyshine. Working symbols: , , , , . A thin roof and a large solid angle Ω make skyshine. McGinley's k ≈ 0.025 m² is a first look; NCRP 151 is geometry-richer.
Purpose
Live realistic example
In symbols
Calculator
Inputs
Outputs
- Skyshine dose rate \dot H0.889 µSv/h
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Narration of this film
A roof, a sky hemisphere, a point in the car park.
A thin roof and a large solid angle Ω make skyshine. McGinley's k ≈ 0.025 m² is a first look; NCRP 151 is geometry-richer.
Watch on YouTube