At 09:05 AM 8/3/2006, Dave Fuller wrote:
>For a given distance D to the antenna the field strength is proportional
>to 1/D(squared). In other words double the distance and you reduce
>field strength by 4. Will be different for "near field" areas....not
>sure how far that is for a typical HF system.
The near field for a HF antenna is surprisingly large, and doesn't have a
lot to do with the physical size of the antenna. The classic (and somewhat
arbitrary) definition of "near field" is the volume within which the
energy stored in the fields around the antenna is greater than or equal to
the energy radiated away.
Another definition is where the ratio of the E and H fields is equal to
free space impedance (377 ohms). For a small antenna (where size of antenna
is much less than a wavelength), this is roughly at wavelength/(2 pi). A
small magnetic loop would follow this sort of rule. However, something as
simple as a dipole violates the assumption inherent in this.
This definition is handy in the RF safety and EMI/EMC complianceworld,
because it sets the boundary where you can just measure E or H, and not
have to worry abou the other (because the ratio is fixed). In the EMI/EMC
area, you're usually not worried about power density, per se, but E field
or H field, depending on the vulnerability of the victim circuit. In the RF
safety world, power density is the important thing, either as a whole body
absorbed energy or a peak absorption in a small volume.
Generally, one divides the volume around the antenna into three categories:
Reactive near field (where the dominant process is one of energy storage),
radiative near field (where radiation is starting to be the dominant
process) and the far field (where it's all radiation). The reactive near
field is where if you put something, it screws up the pattern, because
you're changing the energy flow in and around the antenna. The radiating
near field is less sensitive, but really, it's where you can't make a plane
wave assumption for propagation (that is, power doesn't fall off as 1/r^2)
Where you can get tangled up is in a gain antenna which has significant
energy stored in the field (which applies to just about all Yagis). If you
consider an antenna with an "antenna Q" of, say, 10 (which isn't all that
high), that means that 10 times as much energy is stored in the field as is
radiated away. Fortunately, that energy is spread out within the antenna
volume, so it's not like you'd have to multiply the far field numbers
(which is the "radiated away" part) by 10.
A good example of a system with a LOT of energy stored in the near field,
but radiating fairly little in the far field, is a Tesla coil (which is
really just a LC tank where the C is the capacitance of the coil to
ground). You'd have to be pretty far away from the tesla coil to get to a
distance where the radiated field (which is pretty small) is equal to the
stored field (which is pretty big).
Here are some (conservative) rules of thumb for the boundaries, all based
on D being the largest dimension of the antenna (diagonally across a Yagi!):
The reactive near field is out to r = 0.62 Sqrt(D^3/lambda).
The radiating near field out to 2*D^2/lambda.
The farfield exists beyond 2 D^2/lambda.
Looking at a typical yagi with elements roughly a half wavelength long, and
on a half wavelength boom, we'd take D as 0.707 lambda
(diagonal!).. Plugging in the numbers:
Reactive near field to 0.62*sqrt( (.707^3) * Lambda^2) = 0.62*lambda *
.707^3/2, or, about 0.36 lambda
radiating near field out to 2 * .707^2*lambda^2/lambda or 1 wavelength
far field beyond a wavelength.
The takehome message here is that if you're calculating field strengths,
you can only use the far field approximation (i.e. doubling the distance is
1/4 the power density) if you're a least a wavelength away. A 20m 3
element yagi on a 70 foot tower just meets this. If you're any closer,
then you need to really look at the near fields using something like NEC.
http://home.iae.nl/users/bergervo/gouy/dipole.html has some fascinating
movies of the fields around a dipole
Jim
>
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