He means that the curvature of both the surface and wavefront is assumed
to be small enough on the scale of a wavelength that ray optics is
applicable locally--i.e. that diffraction is not important in most places.
This is a standard move in asymptotic theories. For instance, when you
derive the Stirling series for the gamma (factorial) function, you start
with an integral relationship for gamma(x), do a Taylor expansion for x'
epsilon (epsilon assumed small), integrate term by term, and then let
epsilon go to infinity so that the upper limit of the integral goes
away. At different times you assume that epsilon is very small, and
then that it's infinity. This works because the size of the
contribution from large epsilon is actually negligible--smaller than any
term in the asymptotic series, as x -> infinity. It's fun once you get
used to it.
thanks, for the reply. Ok please consider this following diagram which
shows multple interactions of rays with the body:
http://i34.tinypic.com/29up1l0.jpg
Let's say the ray going from 1 to 2 is associated with plane wave. It
strike s sharp edge at point 2, undergoes diffraction and one of the
ray 2 to 3 hits a triangular facet and undergoes reflection at point
3. Let's say I want to calculate field at 4.
If field at 1 is suppose E1. Then since ray from 1 to 2 is plane
wave :
E(2) = E(1) * exp(-jks12) . This is by formula 1 of first post.
where s12 is distance between 1 and 2 and E(2) is field incident at
point 2.
When plane wave undergoes diffraction at the edge, it results in a set
of conical wave. Let's say one of the ray is 2 to 3.
field incident at 2 = E(2), let D= Diffraction coefficient, s23 =
Distance betwee. So field incident at 3
E(3) = D * E(2) * exp(-jks23) / sqrt(s23). This is by formula 3 of
first post.
or do you think it should be
E(3) = E(2) * exp(-jks23) as we consider all waves locally plane ??
Then I don't understand the purpose behind the thesis mentioning the
other formulas. Is it for far field ? But anyway let us assume the
first formula for E(3) is correct and proceed.
The ray 2-3 hits a facet and undergoes reflection. Now here I get
stuck up because if the incident wave is cylindrical wave, then I do
not know what would be the nature of reflected ray. IF it is a
cylindrical wave again, I need to change formula 1 in first post to
accomodate for 1/sqrt(s) attenuation instead of the 1/s attenuation
factor I had written (which was for spherical wave). This is what
leads to too many questions like what to do when cylindrical
wave/"ray" had hit another edge etc like the one I asked in first
post. However none of this is a problem if you assume all such waves
are plane wave. In that case:
Field at 2 is E(2) = E(1)exp(-jks12). Field at 3 is E(3) = E(2) *
exp(-jks23) and field at 4 is E(4) = E(3) * exp(-jks34).
We are not concerned at all with nature of the wave.
What I find confusing here is that this actually means that the field
has not changed from 1 to 4 if we consider all waves locally plane.
While this might be true if these distances 1-2 2-3 3-4 are pretty
small but it may not be true if object is pretty huge like a
helicopter or something. eg: A ray diffracted from the wings may
travel a few meters before it hits some other surface of helicopter.
Also I the question I asked previously i.e why the thesis mentions
other formulas at all. I have one book on GTD by graeme L james and he
calculates a divergence factor only in case of reflection(the formulas
for diffraction and plane wave remain same). His formula is :
E(s) = Einc * R * DF * exp(-jks)
R is reflection coefficient
DF is divergence factor
E(0) is electric field incident at the point of reflection
s is distance from the point of reflection along the reflected ray at
which we are interested in calculating E(s) field.
k is wavenumber
DF in case of reflecting wavefront being spherical is 1/s, in case
for cylindrical its 1/sqrt(s) and I guess for plane wave it is 1. In
his book he used some complicated derivation for divergence factor for
curved surfaces etc but I don't know how to do it with plane facets.
Any way the formula in his book is :
DF = p1p2 / (p1 + s) (p2 + s)
where s is distance from point fo reflection, p1 and p2 are principal
radii of curvature.
I can figure out the DF in case of incident spherical wave though.
This is because the outgoing wavefront or the reflected wavefront will
also be spherical and you can find the origin for the reflected
spherical wavefront by extending the reflected ray by same distace
behind the facet that the origin of the incident ray is in front of
the facet.(same thing we do with the plane mirrors, here we assume
that the facet act as a mirror) :
http://i36.tinypic.com/2me4qpt.jpg
Now we know the field which was incident on the facet say at some
point 1 because of some incident ray. We know the distance between 1
and O, so the field at O is obviously field at 1 multiplied by field
at 1 and distance between 1 and O. (electric field is attenuated by 1/
distance along spherical wave). Using field at O we can determine
field at any point along the reflected ray based on distance between O
and that point.
GTD and PTD put that case in by hand, by adding "diffracted rays".
Well, what I usually do is trace the rays (and their children rays) as
they come and add up their contributions to electric fields.
Yep. Once you have a diffracted ray, you treat it like any other ray.
Pure ray optics is an asymptotic theory for lambda->0. Roughly
speaking, GTD takes it one more perturbation order, and PTD one more
order after that.
Cheers,
Phil Hobbs
Ok what if I want to find out thescatered electric field in the far
field of the object. The far field radiation is spherical and I want
to calculate the scattered field on a sphere of radius R (R is
extremely huge as we are talking about far field radiation), The
emissions coming from the object may be categorised into many groups
like plane wave, spherical wave or diffraction wave. So does that mean
I need to check the type of ray (plane , spherical or diffraction) and
then apply appropirate formulas(1-3) to calculate contribution of this
ray to total far field scattered radiation ?
My ultimate aim is calculate radar cross section of the object. The
formula for RCS being :
RCS = 4 * PI * R^2 * (|Es|)^2 / (|Ei|)^2
where R is the radius of sphere (tending to infinity), Es is total
scattered electric field vector and Ei is the incident electric field
vector.