Hi MJFlash,
May I ask how you derived the formula?
Here in my country we use a different formula for multi lnb position:
Horizontal offset = focal_length * tan(dish_azimuth - new_azimuth)
Vertical offset = focal_length * tan(dish_elevation - new_elevation)
As an example, your satellite dish is a Fortec Star 90cm, which has a focal length of 510mm. The offsets for you are therefore:
Horizontal: 510mm * tan(174.9 - 160.5 [degrees]) = 130 mm
Vertical: 510mm * sin(46.5 - 44.8 [degrees]) = 15.13 mm
At small angle, my approach is close to yours.
But at larger angle, like 30-40 degrees, the difference becomes larger.
Where I come from, we use 180cm dish to receive satellite in the range of 110E, 113E, 124E, 128E, the azimuth difference is in the range of 5-45 degrees,
where the difference between the two formulas in question is large.
As I got the formula from my fellow sat fan here, and I have not got the chance to really verify it using lnb and dish.
What I did was to mathematically prove my formula, and here it goes,
Assume the dish is a parabolic mirror with focal length of f, further assuming the two satellites are A and B and the azimuth difference is t degree between them.
Remember the Gauss formula for geometric optics, 1/p + 1/q = 1/f where p is the distance between object and the mirror, q the distance between the image and the mirror,
and f the focal length and also the magnify factor=q/p
Next, let's draw a pic of A,B, and the parabolic mirror F
Let the distance between A and F be X
Then the length of sub point C of B on line AF line BC=x sin t
and the length of FC=x cos t
Now let's plug the number to the Gauss formula
since 1/BF ? 1/q = 1/f
since BF is very large, 1/BF can be ignored,
q=f
M=q/p=f/p=f/FC=f/(x cos t)
so we have the final formula:
the image of B is at B' whose position relative to the focal point =
M*p=f/(x cos t) * x sin t
=f tan t
I am here to verify the correctness of my proof and so the correctness of the formula regarding the position of the second lnb to the original lnb.
Thanks.