INGENIA

RAD-30

Buildup factor

Scatter in broad beam.

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Radiationbuildup

Governing equation

I=BI0eμxI=B I_0 e^{-\mu x}

where

I_0
I0 ()
B
Buildup ()
\mu
μ (1/cm)
x
x (cm)
I
I ()

Lecture brief

Historical brief

Beer attenuation, Compton (1923), Klein–Nishina, Bragg–Gray cavity and KERMA are the transport of photons and charged particles in matter. The sheets compute fluence, kerma and stopping. This sheet (RAD-30 — Buildup factor) is the form associated with buildup. Working symbols: I0I_0, BB, μ\mu, xx \rightarrow II. Scatter in broad beam.

Purpose

Purpose: compute II from I0I_0, BB, μ\mu, xx in Radiation physics via I=BI0eμxI=B I_0 e^{-\mu x} Scatter in broad beam. Use it when a real radiation physics question must be answered in SI before a code check.

Live realistic example

In symbols

Live case. Given I0=1.000I_0 = 1.000\,\mathrm{—}, B=2.000B = 2.000\,\mathrm{—}, μ=0.1501/cm\mu = 0.150\,\mathrm{1/cm}, x=10.000cmx = 10.000\,\mathrm{cm}, the governing relation I=BI0eμxI=B I_0 e^{-\mu x} yields I=0.4463I = 0.4463\,\mathrm{—}. Scatter in broad beam. Move a slider: the numbers are this situation, not a canned story.

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Inputs

Outputs

  • I I0.4463
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RAD-30 · dose
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Narration of this film

Scatter in broad beam.

Scatter in broad beam.

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