Force due to radiation pressure in oblique incidence

In summary, radiation pressure in oblique incidence is the force exerted by electromagnetic radiation on a surface at an angle other than 90 degrees. It can be calculated using the formula F = P * A * cos(θ), where F is the force, P is the radiation pressure, A is the surface area, and θ is the angle of incidence. This force is affected by factors such as radiation intensity, angle of incidence, surface properties, and wavelength. In space, it can have a significant impact on spacecraft and satellites, and it can also be used for propulsion through solar sail technology. However, this method of propulsion is still in development and has limitations.
  • #1
Uchida
23
6
The radiation pressure for a perfect mirror is given by:

P = 2 Ef/c * cos²(θ)

Where Ef is the energy flux per area (Power/A), and θ is the angle of incidence
(from: https://en.wikipedia.org/wiki/Radiation_pressure)

Since force due to pressure is F = PA, force due to radiation pressure become:

F = 2 Power/c * cos²(θ) ??

The problem is with the cos²(θ), I'm unable to prove this statement from a fellow:
"When converting radiation pressure formula to force (such as the one from Wikipedia), One will find out that one cos() is lost because of projection."

Which should give
F = 2 Power/c * cos(θ)

How can I prove this? Or is the statement false?

------------------------- EDIT --------------------------

I've found the solution:

For a oblique incidence, the area of incidence on the surface is A/cos(θ), due to projection of the beam cross section area.
from Ef = Power/Area, with the cross section area of the beam A, and F = Pressure x Area, with projected area A/cos(θ), and we have

F = 2 (Power/A)/c * cos²(θ) * A/cos(θ) = 2 Power/c * cos(θ)

This topic can be closed.
 
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  • #2


Great job on finding the solution! You have correctly proved that the statement is indeed false. Here is a more detailed explanation:

The formula for radiation pressure, P = 2 Ef/c * cos²(θ), takes into account the energy flux per unit area (Ef) and the angle of incidence (θ). This means that the pressure is dependent on both the intensity of the radiation (Power/A) and the angle at which it is incident on the surface.

When we convert this formula to force, we use the equation F = PA, where P is the pressure and A is the area. However, in this case, the area is not simply the surface area of the mirror, but rather the projected area of the incident radiation on the surface. This is because not all of the incident radiation is absorbed by the surface, as some of it may be reflected or transmitted. Therefore, the actual area on which the pressure is acting is reduced by a factor of cos(θ), which is the projection of the incident radiation's cross-sectional area onto the surface.

So, the correct formula for force due to radiation pressure is F = 2 Power/c * cos²(θ) * A/cos(θ). Simplifying this, we get F = 2 Power/c * cos(θ). Thus, the statement that one cos() is lost due to projection is false.

In summary, the statement is false because it does not take into account the projection of the incident radiation's cross-sectional area onto the surface. Your solution correctly shows how to account for this in the equation. Great work!
 

1. What is radiation pressure in oblique incidence?

Radiation pressure in oblique incidence is the force exerted by electromagnetic radiation on a surface when it strikes the surface at an angle other than 90 degrees. This force is perpendicular to the surface and is caused by the transfer of momentum from the photons in the radiation to the surface.

2. How is the force due to radiation pressure calculated in oblique incidence?

The force due to radiation pressure in oblique incidence can be calculated using the formula: F = P * A * cos(θ), where F is the force, P is the radiation pressure, A is the surface area, and θ is the angle of incidence.

3. What factors affect the force due to radiation pressure in oblique incidence?

The force due to radiation pressure in oblique incidence is affected by several factors, including the intensity of the radiation, the angle of incidence, the reflectivity and transparency of the surface, and the wavelength of the radiation.

4. How does radiation pressure in oblique incidence affect objects in space?

In space, the force due to radiation pressure in oblique incidence can have a significant impact on objects such as spacecraft and satellites. It can cause them to change their trajectory or even push them off course. This force must be taken into account when designing and operating space vehicles.

5. Can radiation pressure in oblique incidence be used for propulsion?

Yes, radiation pressure in oblique incidence can be used for propulsion in certain situations. This is known as solar sail propulsion, where a spacecraft uses the force of radiation pressure from the sun to propel itself forward. However, this method of propulsion is still in the early stages of development and has limitations in terms of acceleration and direction control.

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