How Does Energy Disperse from a Finite Line Source?

This transition occurs at a distance x measured 90 degrees from the center of the line source. In summary, the principles of energy dispersion from a point source and an infinite line source follow the inverse square law and ½ inverse square law respectively, and for a finite line source, the energy dispersion transitions from an inverse square law to a ½ inverse square law at a certain distance from the source.
  • #1
jlenard
4
0
Inverse square law

Does anyone have an absolute basic understanding of
"first order principles of energy dispersion"

(A) Energy from a point source disperses spherically
at the inverse square law.
(B) Energy from an infinite line source disperses cylindrically
at ½ inverse square law.

Question?
What is the energy dispersion from a finite line source?

Measured 90deg from center of line source, at distance x, where transition from ½ inverse square law, back to, inverse square law, takes place.

Can anyone throw light on this question without diversions?
1 First order principles only.
2 In space, zero boundaries.
3 Line length magnitudes greater than any wavelength of energy dispersed.

Thank you.
 
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  • #2
Answer: Energy from a finite line source disperses cylindrically at the inverse square law until it reaches the point where the distance from the source is equal to the length of the line source. At this point, the energy dispersion transitions from an inverse square law to a ½ inverse square law.
 

What is the inverse square law?

The inverse square law is a physical principle that states that the intensity of a physical quantity (such as light, sound, or gravity) decreases in proportion to the square of the distance from the source.

What is the formula for the inverse square law?

The formula for the inverse square law is I = k/d^2, where I is the intensity, k is a constant value, and d is the distance from the source.

How does the inverse square law apply to light?

In the context of light, the inverse square law states that the brightness of a light source decreases as the square of the distance from the source increases. This means that the further you are from a light source, the dimmer it will appear.

Why is the inverse square law important?

The inverse square law is important because it helps us understand and predict how physical quantities, such as light and sound, behave as they move away from their source. It is also used in various fields of science, such as astronomy and physics, to make calculations and predictions.

What are some real-life examples of the inverse square law?

Some real-life examples of the inverse square law include the brightness of a light bulb, the strength of a radio signal, and the force of gravity between two objects. It also applies to phenomena such as sound waves and radiation.

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