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Radiant Flux

Storyboard

The light is irradiated, that is to say it flows so that the fundamental magnitudes refer to the amount of photons that are emitted, cross a section or are absorbed.

Since the amount of photons in a color is proportional to the energy, the flow is proportional to the energy per time, that is, the power.

>Model

ID:(297, 0)



Decrease in intensity with distance

Image

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If we think of light as a flow of photons, they will move away from their source and spread over an increasingly larger surface:

In this way, the intensity decreases as we move away from the source, diminishing inversely with the square of the distance.

ID:(1664, 0)



Brightness of Light by Hole

Description

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When light passes through the aperture, the intensity depends on the angle of the beam relative to the original direction of the beam, denoted as \theta.

The intensity I is given by

I(r,\theta)=\displaystyle\frac{r_0^2}{r^2}I_0\cos\theta

\theta
Angle of Propagation
rad
5139
r
Distance to Source
m
5137
I
Light Intensity
W/m^2
5140
L
luminosity
Cd
5138
I_r =( r_0 ^2/ r ^2) I_0 r_1r_2I_1I_2

ID:(3352, 0)



Light travelling through an Slite

Image

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When light passes through an aperture, it begins to disperse. Its intensity decreases both with the distance from the aperture and with the angle relative to the original direction of propagation:

ID:(1861, 0)



Light Intensity with Distance

Equation

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Since photons are distributed over an area of size 4\pi r^2, the number per unit area of these photons decreases. As the number of photons per unit area is the density, it reduces as follows:

I_r =\displaystyle\frac{ r_0 ^2}{ r ^2} I_0

r_1
Distancia a la fuente 1
m
9829
r_2
Distancia a la fuente 2
m
9830
I_1
Intensidad de la luz 1
W/m^2
9831
I_2
Intensidad de la luz 2
W/m^2
9832
I_r =( r_0 ^2/ r ^2) I_0 r_1r_2I_1I_2

Intensity is measured in candelas (cd), which is the amount of light emitted by an object at a temperature of 2042.5 K over an area of size 1/600000 m^2.

ID:(3191, 0)