Please help with calculation involve solid angle.

In summary, the example presented is a problem involving the calculation of the ratio of solid angles for the planet Mars at a specific wavelength and measured with a specific radio telescope. The book's answer to the problem involves a correction factor of π/4, which may be due to the concaveness of the planet's surface. However, the book does not mention this and the author has not been able to confirm the answer using a cosine calculator. There is also a question about the interpretation of the antenna's HPBW as a square instead of a circle. The underlying physics of EM radiation at this specific wavelength and its behavior on the Martian surface is also uncertain.
  • #1
yungman
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This is only an example from Kraus Antenna 3rd edition page 404. The question is really a math problem involves calculation of ratio of solid angles. Just ignore the antenna part. this is directly from the book:

Example 12-1.1 Mars temperature

The incremental antenna temperature for the planet Mars measured with the U.S. Naval Research Lab 15-m radio telescope antenna at 31.5mm wavelength was found to be 0.24K(Mayer-1). Mars subtended an angle of 0.005 deg at the time of the measurement. The antenna HPBW=0.116 deg. Find the average temperature of the Mars at 31.5mm wavelength.

The answer from the book:

[tex]T_s=\frac {\Omega_A}{\Omega_S}\Delta{T_A}\;\;\approx\;\frac {0.116^2}{\frac{\pi}{4}0.005^2}(0.24)=164K[/tex]



I don't understand where the [itex]\frac {\pi}{4}[/itex] in the denominator comes from. This is just a simple problem where the ratio of the area of two disk one with Θ=0.116/2 and the other with Θ=0.005/2. I try to use the following to calculate:

[tex]\Omega=\int_0^{2\pi} d\phi\;\int_0^{\theta/2}\sin {\theta} d \theta[/tex]

So

[tex]\frac{\Omega_A}{\Omega_S}\;=\;\frac{\int_0^{2\pi} d\phi\;\int_0^{0.116/2}\sin {\theta} d \theta}{\int_0^{2\pi} d\phi\;\int_0^{0.005/2}\sin {\theta} d \theta}\;=\;\frac{2\pi\int_0^{0.116/2}\sin {\theta} d \theta}{2\pi\int_0^{0.005/2}\sin {\theta} d \theta}[/tex]

[tex] \frac{\Omega_A}{\Omega_S}\;=\;\frac{(1- 0.999999487)}{(1-0.999999999)}=538.2[/tex]

But using the answer from the book:

[tex]\frac{0.116^2}{\frac{\pi}{4}0.005^2}\;=\;685.3[/tex]

I just don't get the answer from the book. Can it be the limitation of my calculator to get cos 0.0025 deg? Can anyone use their calculator to verify the number? please help.

Thanks

Alan
 
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  • #2
I'll take a guess at this. It seems like the same idea as "geometric form factors" in radiative heat transfer.

The telescope is "seeing" a piece of space that you can take as a flat disk (diameter 0.116 degrees)

But the surface of Mars that is radiatiing is not a flat disk, it is a hemisphere. The "brightness" as seen by the telescope will be maximum in the center and less at the edges.

That will give you another factor of ##\sin\theta## or ##\cos\theta## in the integral for Mars. Probably the "correction factor" of ##\pi/4## is a well known result, since most astronomical objects are approximately spherical.
 
  • #3
Thanks for you time. I don't mean to say you are not right as it might well can be. On the first pass, I don't think that's what the book meant, the reason is, this example is right at the beginning of the chapter and the book did not mention anything about the concaveness of the star. Also the answer of the book:

[tex]T_s=\frac {\Omega_A}{\Omega_S}\Delta{T_A}[/tex]

Which does not contain any compensation for the concaveness of the planet. So far, this book has been pretty straight forward and concise. I type out the exact words from the book in my post and nothing about this. I scan through the later part of the chapter and there's nothing about this either. Basically it only talked about the ratio of the solid angle for object smaller than the half power angle.

Again thank you for your time. I manage to go on line and use a cosine calculator that don't flag error of 0.0025 deg and gave me 2 more digits in the decimal place than my calculator, the answer is even more off! So I don't think the small angle is the cause of the problem.
 
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  • #4
AlephZero said:
But the surface of Mars that is radiatiing is not a flat disk, it is a hemisphere. The "brightness" as seen by the telescope will be maximum in the center and less at the edges.
Are you sure about that? It doesn't seem right to me.
yungman, is it possible that HPBW is to be interpreted as a square, not a circle?
 
  • #5
haruspex said:
Are you sure about that? It doesn't seem right to me.
yungman, is it possible that HPBW is to be interpreted as a square, not a circle?

It kind of make sense as the surface is concave and you have the max reflection at the center of the planet where the surface is true normal to the propagation. But as I said, the equation don't reflect this, all it gave was the ratio of the two solid angle where there is no reason for the π/4 to appear.

That I am pretty sure, the main lope a very directional antenna is like a long balloon or sausage! But still don't explain the pi/4 even if you look at it as square.
 
  • #6
yungman said:
It kind of make sense as the surface is concave and you have the max reflection at the center of the planet where the surface is true normal to the propagation.
Seems to me the model is to suppose the surface is uniform temperature and is radiating on that basis. I believe a sphere at uniform intrinsic brightness would appear appear as a uniformly bright disc whatever position it is viewed from, but I'm prepared to be proved wrong about that.
That I am pretty sure, the main lope a very directional antenna is like a long balloon or sausage!
Yes, but what I'm suggesting is that when an antenna is quoted as having a diameter of such-and-such, that is to be interpreted as the square root of the 'effective' area, whatever shape and response pattern the actual area is. I've no idea whether this is the case - just trying to make sense of the equation
 
  • #7
haruspex said:
Are you sure about that? It doesn't seem right to me.

I'm not sure either, whcih is why I started my post with "I'll take a guess at this".

The physics question here is whether each point on the surface of Mars radiates energy in all directions like a "point source", or whether some effect (e.g. electrical conductivity of the Martian material) means sonething different happens. It's not self-evident to me that EM radiation with wavelength 31.5mm would behave the same way as visible light (the wavelengths are different by a factor of 10^6) but I don't know whether it does or it doesn't.
 
  • #8
haruspex said:
Seems to me the model is to suppose the surface is uniform temperature and is radiating on that basis. I believe a sphere at uniform intrinsic brightness would appear appear as a uniformly bright disc whatever position it is viewed from, but I'm prepared to be proved wrong about that.

Yes, but what I'm suggesting is that when an antenna is quoted as having a diameter of such-and-such, that is to be interpreted as the square root of the 'effective' area, whatever shape and response pattern the actual area is. I've no idea whether this is the case - just trying to make sense of the equation

Thanks for the answer. In the whole, they use round shape like a cone to represent the main lobe. I don't believe the book mean square. Besides, using square don't explain ∏/4 either.

The question is whether I am doing it right with my approach assuming the Mars has uniform temperature on the surface. I really believe the book is wrong to put the ∏/4 in. The square of the degree will be good already as the ratio is the same using Sr or degree.

I just try taking my result (538) divide by ∏/4, the answer is 685 which is the same as the book!
 
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  • #9
yungman said:
Besides, using square don't explain ∏/4 either.
Yes it does. If the antenna 'diameter', A, is interpreted as the side of a square then its area is A2. Mars' diameter, M, gives an area πM2/4.
 
  • #10
Yes, is the only way to for it to make sense. I just don't know of any antenna that have a square cross section beam. Mostly has round or at least roundish cross section. I guess we never know what the author think. Anyway, thanks for the help.
 
  • #11
yungman said:
I just don't know of any antenna that have a square cross section beam.
I'm sure they don't, but it's quite possible that the apertures are conventionally quoted as though they are square. In other words, it is not saying it is actually width D, merely that the effective area is D2.
 
  • #12
Thanks for your help.

Alan
 

FAQ: Please help with calculation involve solid angle.

1. What is solid angle?

Solid angle is a measure of the amount of space an object takes up in three-dimensional space. It is measured in steradians and is analogous to how angles measure the amount of space an object takes up in two-dimensional space.

2. How is solid angle calculated?

Solid angle is calculated by dividing the area of a sphere subtended by the object by the square of the radius of the sphere. It can also be calculated by dividing the length of the arc of the object on the surface of the sphere by the radius of the sphere.

3. What is the difference between solid angle and regular angle?

The main difference between solid angle and regular angle is the dimensionality of the space being measured. Regular angles measure the amount of space in two-dimensional space, while solid angles measure the amount of space in three-dimensional space.

4. Why is solid angle important in science?

Solid angle is important in science because it is used to measure the amount of radiation that passes through a specific area, such as in astronomy and optics. It is also used in the calculation of electric and magnetic fields, as well as in the study of solid-state physics and quantum mechanics.

5. Are there any practical applications of solid angle?

Yes, solid angle has many practical applications in various fields. In architecture and lighting design, it is used to calculate the amount of light that will be emitted from a light source in a specific direction. In geology, solid angle is used to measure the surface area of crystals. In computer graphics, it is used to determine the viewing angle of a virtual object.

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