INGENIA

RPR-13

Skyshine snapshot

Ḣ = k Ḣ0 B Ω / d². Roof scatter raining down outside the vault.

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ScatterNCRP 151 skyshine

Governing equation

H˙=kH˙0BΩ/d2\dot H=k\dot H_0 B\Omega/d^{2}

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 ()
\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: H˙0\dot H_0, BB, Ω\Omega, dd, kk \rightarrow H˙\dot H. 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

Purpose: compute H˙\dot H from H˙0\dot H_0, BB, Ω\Omega, dd, kk in Radiation protection via H˙=kH˙0BΩ/d2\dot H=k\dot H_0 B\Omega/d^{2} Ḣ = k Ḣ0 B Ω / d². Roof scatter raining down outside the vault. Use it when a real radiation protection question must be answered in SI before a code check.

Live realistic example

In symbols

Live case. Given H˙0=200.000mSv/h\dot H_0 = 200.000\,\mathrm{mSv/h}, B=0.050B = 0.050\,\mathrm{—}, Ω=0.800sr\Omega = 0.800\,\mathrm{sr}, d=15.000md = 15.000\,\mathrm{m}, k=0.025m2k = 0.025\,\mathrm{m^{2}}, the governing relation H˙=kH˙0BΩ/d2\dot H=k\dot H_0 B\Omega/d^{2} yields H˙=0.889μSv/h\dot H = 0.889\,\mathrm{\mu Sv/h}. A roof, a sky hemisphere, a point in the car park. Move a slider: the numbers are this situation, not a canned story.

Calculator

Inputs

Outputs

  • Skyshine dose rate \dot H0.889 µSv/h
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RPR-13 · dose
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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.

Reading speed

Watch on YouTube