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#1
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OH, for Pete's sake. Loops are sensitive to the H vector. Wires receive
the E vector. Most near field noise tends to be predominantly E field. But, that seems to only be effective up to 3 or 4 MHz, due to the wavelength factor, i. e. the near field shrinks as you go higher in frequency. Fully formed far field wavefronts of noise sources will be just like wanted signals, and unless some polarization difference is available, then directivity is the only way to improve S/N. Only in special circumstances can you see much improvement above 5 MHz due to near field/far field differentiation. But, my point was that no improvement in S/N was reported in the original post. Only a decrease of noise accompanied by a decrease in signal. No relative comparison offered. Are we supposed to *assume* that the signals went down due to time of day, while the noise went down because it is a loop? Maybe the opposite is true? Not enough data to prove either. -- Crazy George Remove N O and S P A M imbedded in return address |
#2
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![]() But, that seems to only be effective up to 3 or 4 MHz, due to the wavelength factor, i. e. the near field shrinks as you go higher in frequency. REALLY? How does it do that? W4ZCB |
#3
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Say, for purposes of illustration, that the near field ends at 1 wavelength.
At 2 MHz, that is very roughly 530 feet . At 14 MHz it is about 64 feet. At 30 MHz, it has shrunk to ~32 feet. -- Crazy George Remove N O and S P A M imbedded in return address "Harold E. Johnson" wrote in message news:Qf_Ic.82101$Oq2.21575@attbi_s52... But, that seems to only be effective up to 3 or 4 MHz, due to the wavelength factor, i. e. the near field shrinks as you go higher in frequency. REALLY? How does it do that? W4ZCB |
#4
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![]() "Crazy George" wrote in message ... Say, for purposes of illustration, that the near field ends at 1 wavelength. At 2 MHz, that is very roughly 530 feet . At 14 MHz it is about 64 feet. At 30 MHz, it has shrunk to ~32 feet. -- Why would the near field end at 1 wavelength? It ends when the wave front arriving at the receiving antenna becomes planar. ie, to function efficiently in the far field, the receiving antenna needs to intercept a planar wavefront. That is, the individual rays need to be arriving in parallel. If the distance between antennas is very great, that is very nearly the case. If the capture area of the receiving antenna is great relative to the distance to the source, the received energy arrives as non parallel rays that basically reach the receiving antenna out of phase with each other and partially cancel. So, the gain of antennas measured in the "near field", where the received energy is not a planar wavefront, will be in error. The distance to the end of the near field is highly dependent on the gain of the antenna and with UHF and SHF antennas often exhibiting very high gain, their near fields can be and often are very large. The power collected by a receiving antenna within the transmitters near field is very nearly constant with distance. In the far field, recovered power varies inversely with the square of the distance. Regards W4ZCB |
#5
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Harold E. Johnson wrote,
It ends when the wave front arriving at the receiving antenna becomes planar. ie, to function efficiently in the far field, the receiving antenna needs to intercept a planar wavefront. That is, the individual rays need to be arriving in parallel. If the distance between antennas is very great, that is very nearly the case. If the capture area of the receiving antenna is great relative to the distance to the source, the received energy arrives as non parallel rays that basically reach the receiving antenna out of phase with each other and partially cancel. So, the gain of antennas measured in the "near field", where the received energy is not a planar wavefront, will be in error. The distance to the end of the near field is highly dependent on the gain of the antenna and with UHF and SHF antennas often exhibiting very high gain, their near fields can be and often are very large. Balanis divides the near-field region into two parts: a reactive near-field R0.62 square root(D^3/Lambda) where D is the largest antenna dimension, Lambda is the wavelength, and R is the distance from the antenna surface, and a radiating near-field region R2D^2/Lambda. The far-field he defines as anything greater than 2D^2/Lambda. He gives exceptions to these rules, so take them with a grain of salt. 73, Tom Donaly, KA6RUH |
#6
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#7
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Hi William, All,
As is common with comparisons, the problems arise due to the shifting sand these arguments are built upon. On Wed, 14 Jul 2004 12:09:17 -0400, William Mutch wrote: But, my point was that no improvement in S/N was reported in the original post. True; I didn't report it but it is there. Typically at most frequencies the desired signal is reduced 1 to 2 S-units with respect to the whip antenna (strong ones) or my high long wire weaker signal...156 feet AWG 16 up 45 feet fed off center w/ a 4:1 balun) but the noise level is reduced by anywhere from 3 to 6 S-units...a very! worthwhile tradeoff. Presumably, the comparison is loop vs. these others. It is not explicit and that is one of the problems of reporting and subsequent interpretation - hence the observation in the double quote above. However, the "issue" is more has anything really changed? A loop (dipole) compared to two verticals. Arguably the so-called off center fed long wire is presumed to be a dipole, however (again poor reporting) nothing says of this antenna being choked. Lacking that choke offers every inducement of Common Modality (the antenna is, after all, fully and admittedly unbalanced by its very description). Common Modality is ever bit a noise hazard as any vertical (is supposed to be - another nightmarish fantasy under the bed). Hence, any perceived boon of noise reduction comes as a consequence of the loop's faithfully performing as a - dipole! Wonders never cease. Exact quantitative measurements are not possible on the Sat800 RCVR because you can't turn off the AGC. I don't know how this got started as a unnecessary evil - AGC is what drives the S-Meter. AGC is only an issue if you want to derive signal strength via modulation levels - which nobody here does anyway. My understanding of why the shielded loop performs this way is that near field noise is cancelled while far field signal is only attenuated by some factor relating to capture area. In my temporary rooftop mount I was unable to easily check out the effect of broadside null. Tom has posted in this thread very simple metrics to obtain just what constitutes near field. The incantation of near/far fields belies simpler explanations. If there is any issue of noise that relates to its nearness, it follows that you are the source. You being the source means that you also have the capacity to correct (and building a magic antenna is possibly the most superstitious response to that problem). The loop simply has less coupling (and less signal - that means there is a constant of proportionality in S/N) than a full sized dipole sitting over this noisy domicile. I have a random wire antenna that passes within 2 feet of an 80W Fluorescent fixture with a humming ballast. I barely pull in S-1 worth of noise and a loop would stand to do worse at that same distance. If I find that little noise troublesome, I turn off the noise. The fact that the shielded loop performs as a dipole is proof of its efficient construction (many fail to achieve even this). There is very little more that can be said about its qualities short of its loss of sensitivity. 73's Richard Clark, KB7QHC |
#8
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![]() "William Mutch" schreef in bericht the shielded loop performs this way is that near field noise is cancelled while far field signal is only attenuated by some factor relating to capture area. In my temporary rooftop mount I was unable to easily check out the effect of broadside null. William, I have done some work on local QRM reduction during the last few years. Summarized on: http://home.plex.nl/~jmsi/ Most important is avoiding any coupling with the coax/feedline. With small magnetic loops this is easy to accomplish and my guess is that this is why loops are less susceptible for local QRM. That is why I choose small loops instead of small dipoles. 73 de Jan PA0SIM |
#9
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On Tue, 13 Jul 2004 17:57:21 -0500, "Crazy George"
wrote: OH, for Pete's sake. Loops are sensitive to the H vector. Wires receive the E vector. Most near field noise tends to be predominantly E field. But, that seems to only be effective up to 3 or 4 MHz, due to the wavelength factor, i. e. the near field shrinks as you go higher in frequency. Fully formed far field wavefronts of noise sources will be just like wanted signals, and unless some polarization difference is available, then directivity is the only way to improve S/N. Only in special circumstances can you see much improvement above 5 MHz due to near field/far field differentiation. In the _far_ field both the E and H fields are inversely proportional to distance and have the 120 pi (377 ohm) relation (impedance) between the fields. However, in the _near_field_ ( 1 lambda) the 377 ohm relationship is no longer valid and the magnetic field is inversely proportional to the square of the distance, while the electric field is inversely proportional to the cube of distance. Summarising the graph from an article by Lloyd Butler VK5BR in Amateur Radio, August 1990: The output voltages from both E and H field antenna system are calibrated to the same value at 1 lambda (i.e. in the far field). The antennas are moved closer, when the E and H antennas are moved to 0.05 lambda, the E antenna delivers 50 dB and the H antenna 40 dB (relative to 1 lambda) i.e. the H-field is 10 dB quieter. At 0.005 lambda, the E field antenna output is 110 dB and the H-field 80 dB, i.e. the H field antenna is 30 dB is quieter. Thus, with same far field sensitivity, the sensitivity to very local interference is attenuated considerably when _only_ the H field is used. However, at 3.5 MHz and 80 m wavelength, 0.05 lambda corresponds to 4 m and 0.005 lambda to 40 cm, so we are talking about really close noise sources. At even higher frequencies the number of potential interference sources is dropping within the 0.05 (or even 0.1) lambda radius from the receiving antenna, in which the H antenna has an advantage. However, on the 135 kHz LF band (lambda 2.2 km), the distances would be 110 m resp. 11 m, thus much more unwanted interface sources could be eliminated. Shielding the H-loop simply prevents the stronger E field from entering the loop and thus destroying part of the advantage of using the H-antenna. Paul OH3LWR |
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