INGENIA

RAD-29

Inverse square

Point-source fluence.

Reading speed
Radiationinverse square

Governing equation

I=I1(d1/d)2I=I_1 (d_1/d)^2

where

I_1
At d1 ()
d_1
d1 (m)
d
d (m)
I
Intensity ()

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-29 — Inverse square) is the form associated with inverse square. Working symbols: I1I_1, d1d_1, dd \rightarrow II. Point-source fluence.

Purpose

Purpose: compute II from I1I_1, d1d_1, dd in Radiation physics via I=I1(d1/d)2I=I_1 (d_1/d)^2 Point-source fluence. 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 I1=1.000I_1 = 1.000\,\mathrm{—}, d1=1.000md_1 = 1.000\,\mathrm{m}, d=2.000md = 2.000\,\mathrm{m}, the governing relation I=I1(d1/d)2I=I_1 (d_1/d)^2 yields I=0.2500I = 0.2500\,\mathrm{—}. Point-source fluence. Move a slider: the numbers are this situation, not a canned story.

Calculator

Inputs

Outputs

  • Intensity I0.2500
Reading speed

Watch on YouTube

Free library

Full library

Free PDF / open book

YouTube channels

RAD-29 · dose
00:0 / 00:08

Narration of this film

Point-source fluence.

Point-source fluence.

Reading speed

Watch on YouTube