INGENIA

RPR-32

Inverse square with air attenuation

Ḣ(r) = Ḣ0 (r0/r)² e^{−μ(r−r0)}. Distance plus a thin air slab.

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GeometryISL + air attenuation

Governing equation

H˙(r)=H˙0(r0/r)2e−μ(r−r0)\dot H(r)=\dot H_0(r_0/r)^{2}e^{-\mu(r-r_0)}

r∈[0.5,200]r \in \left[0.5, 200\right]

where

\dot H_0
Rate at r0 (µSv/h)
r_0
Reference distance (m)
r
Distance (m)
\mu
Air attenuation μ (1/m)
\dot H
Dose rate (µSv/h)

The figure, part by part

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RPR-32 · dose
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①

Governing law — red

H˙(r)=H˙0(r0/r)2e−μ(r−r0)\dot H(r)=\dot H_0(r_0/r)^{2}e^{-\mu(r-r_0)}

r∈[0.5,200]r \in \left[0.5, 200\right]

r=0.5r = 0.5H˙=401.6\dot H = 401.6

②

Domain of the variable — blue

rmin⁡=0.5,rmax⁡=200r_{\min} = 0.5,\quad r_{\max} = 200

r∈[0.5,200]r \in \left[0.5, 200\right]

r=0.5r = 0.5r=0.5r = 0.5

③

Response curve — green

H˙(r)=H˙0(r0/r)2e−μ(r−r0)\dot H(r)=\dot H_0(r_0/r)^{2}e^{-\mu(r-r_0)}

r∈[0.5,200]r \in \left[0.5, 200\right]

r=0.5r = 0.5H˙=401.6\dot H = 401.6

④

Rate of change — amber

dH˙dr\frac{\mathrm{d}\dot H}{\mathrm{d}r}

r∈[0.5,200]r \in \left[0.5, 200\right]

r=1.755r = 1.755H˙′=−155.7\dot H^{\prime} = -155.7

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-32 — Inverse square with air attenuation) is the form associated with ISL + air attenuation. Working symbols: H˙0\dot H_0, r0r_0, rr, μ\mu →\rightarrow H˙\dot H. Air μ ≈ 0.005–0.01 m⁻¹ for diagnostic x-rays and much smaller for MV / ⁶⁰Co. Scatter in air (skyshine) is a separate term.

Purpose

Purpose: compute H˙\dot H from H˙0\dot H_0, r0r_0, rr, μ\mu in Radiation protection via H˙(r)=H˙0(r0/r)2e−μ(r−r0)\dot H(r)=\dot H_0(r_0/r)^{2}e^{-\mu(r-r_0)} Ḣ(r) = Ḣ0 (r0/r)² e^{−μ(r−r0)}. Distance plus a thin air slab. 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=100.000 μSv/h\dot H_0 = 100.000\,\mathrm{\mu Sv/h}, r0=1.000 mr_0 = 1.000\,\mathrm{m}, r=10.000 mr = 10.000\,\mathrm{m}, μ=0.008 1/m\mu = 0.008\,\mathrm{1/m}, the governing relation H˙(r)=H˙0(r0/r)2e−μ(r−r0)\dot H(r)=\dot H_0(r_0/r)^{2}e^{-\mu(r-r_0)} yields H˙=0.931 μSv/h\dot H = 0.931\,\mathrm{\mu Sv/h}. Expanding spheres with a slow exponential skin. Move a slider: the numbers are this situation, not a canned story.

Calculator

Inputs

Outputs

  • Dose rate \dot H0.931 µSv/h
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RPR-32 · dose
00:0 / 00:08

Narration of this film

Expanding spheres with a slow exponential skin.

Air μ ≈ 0.005–0.01 m⁻¹ for diagnostic x-rays and much smaller for MV / ⁶⁰Co. Scatter in air (skyshine) is a separate term.

Reading speed

Watch on YouTube