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#1
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On Sep 11, 2:53*am, Jon Kåre Hellan wrote:
writes: Roy Lewallen wrote: wrote: Of course. Everyone knows the gain of a parabola is directly proportional to the size in wavelengths, or: G=10*log k(pi*D/L)^2 Where G= gain in DB over an isotropic, k ~ .55 for most real parabolas, D is the diameter, and L is the wavelength (wavelength and diameter in the same units. So a 2,000 foot parabola on 20m would have just about 58db gain. Hm. I get 47. Roy Lewallen, W7EL Hmm, when I use 14 Mhz and 6 decimal places I get 37; must have fat fingered it the first time. Going a different way, I also get about 37. Aperture of a dish is the area, pi*r^2. r is about 14.2 wl, so area is about 635 sq. wl. Aperture of a dipole is 1/4 * 1/2 wl = 1/8 sq. wl. That makes gain 635/(1/8) = 635*8, i.e about 5100 or just over 37 dBd. This assumes 100 % illumination of the dish, which we won't achieve. So make it 35 dBd or so, i.e. 37 dBi. Using the o.p.'s formula, I get 36.5 dBi. * It's odd that pi is squared in the formula. The squared part must be to account for the area of the dish, which is pi*r^2. Obviously, this can has been compensated for by the choice of 'k'. Whoaaa guys............! Let us think a bit more regarding the basics presented instead of parrotting dish's as used in the present state of the art. Isn't a dish built around phase change of a half wave dipole in inter magnetic coupling? If I have a flash light that is focussed does this wavelength aproach still apply? I thought it would be a question of action and reaction. Trow a ball against the wall and it bounces back in a reflective manner to the angle of velocity. A dish as presently used changes the phase of a given signal to reverse it's direction. In physics we can also talk about mechanical force that rebound and rebound has nothing to do with wavelength! If we consider radiation as being the projection of particles instead of wavelike oscillation then surely the size of the reflector is solely based on what can be collected from the emmitter such that it rebounds to a point or a focussed form ? I ask the question as I know nothing about the reflective phenomina of dish's tho I have visited the one in P.R. where the dish is formed with the knoweledge that the radiation spreads out according to the emmiter used and thus when it reaches the reflector the unit strength is weaker which the dish attempts to reverse by refocussing. But then I could be totally in error thus the question to the experts Best regards Art Unwin KB9MZ .. |
#2
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On Thu, 11 Sep 2008 06:18:14 -0700 (PDT), Art Unwin
wrote: If I have a flash light that is focussed does this wavelength aproach still apply? The reflector (or magnifier lens, take your pick) is on order of at least 1 centimeter. The light wavelength is on order of 500 nanometers. Ratio = 20,000:1 Beam is generally no narrower than 15 degrees. At a distance of, say, 6 feet, that beam would cover a diameter of 18 inches. Nothing like a Lazer (sic) if that is the goal. 73's Richard Clark, KB7QHC |
#3
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On Sep 11, 10:37*am, Richard Clark wrote:
On Thu, 11 Sep 2008 06:18:14 -0700 (PDT), Art Unwin wrote: If I have a flash light that is focussed does this wavelength aproach still apply? The reflector (or magnifier lens, take your pick) is on order of at least 1 centimeter. *The light wavelength is on order of 500 nanometers. Ratio = 20,000:1 Beam is generally no narrower than 15 degrees. *At a distance of, say, 6 feet, that beam would cover a diameter of 18 inches. *Nothing like a Lazer (sic) if that is the goal. 73's Richard Clark, KB7QHC I see no basis for the inclusion of wavelengths when one is not using a straight radiator A straight radiator requires one type of reflector an array that is condensed to a smaller volume requires a reflector that is based on the propagation from that radiator. If propagation flares out then you can calculate dish size via WL. If propagation is of a different form then the dish must be designed accordingly.The important factor as I see it is the mode of propagation and what area is required at a distance to account for tha propagation mode. If one starts with a lazer then the reflecting surface need not be larger than the initiating beam area assuming zero scattering. Your thinking is based solely on the state of the art via reading matter. You need to go back in physics to the four forces of the standard model to analyse this question on the basis of the unification theory which is all conclusive where one can determine relative ejection paths from the radiator. The latter may well gyrate to WL I suppose |
#4
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On Thu, 11 Sep 2008 09:38:46 -0700 (PDT), Art Unwin
wrote: On Sep 11, 10:37*am, Richard Clark wrote: On Thu, 11 Sep 2008 06:18:14 -0700 (PDT), Art Unwin wrote: If I have a flash light that is focussed does this wavelength aproach still apply? The reflector (or magnifier lens, take your pick) is on order of at least 1 centimeter. *The light wavelength is on order of 500 nanometers. Ratio = 20,000:1 Beam is generally no narrower than 15 degrees. *At a distance of, say, 6 feet, that beam would cover a diameter of 18 inches. *Nothing like a Lazer (sic) if that is the goal. I see no basis for the inclusion of wavelengths when one is not using a straight radiator Read your own question. There is no such thing as a "straight radiator" of light. There is everything to do with wavelength or you could never see light. 73's Richard Clark, KB7QHC |
#5
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On Sep 11, 2:55*pm, Richard Clark wrote:
On Thu, 11 Sep 2008 09:38:46 -0700 (PDT), Art Unwin wrote: On Sep 11, 10:37*am, Richard Clark wrote: On Thu, 11 Sep 2008 06:18:14 -0700 (PDT), Art Unwin wrote: If I have a flash light that is focussed does this wavelength aproach still apply? The reflector (or magnifier lens, take your pick) is on order of at least 1 centimeter. *The light wavelength is on order of 500 nanometers. Ratio = 20,000:1 Beam is generally no narrower than 15 degrees. *At a distance of, say, 6 feet, that beam would cover a diameter of 18 inches. *Nothing like a Lazer (sic) if that is the goal. I see no basis for the inclusion of wavelengths when one is not using a straight radiator Read your own question. *There is no such thing as a "straight radiator" of light. *There is everything to do with wavelength or you could never see light. 73's Richard Clark, KB7QHC If you say so and are comfortable with that then stick with it ! My thoughts are with the reflector and it's design |
#6
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On Thu, 11 Sep 2008 13:21:15 -0700 (PDT), Art Unwin
wrote: Read your own question. *There is no such thing as a "straight radiator" of light. *There is everything to do with wavelength or you could never see light. If you say so and are comfortable with that then stick with it ! My thoughts are with the reflector and it's design Let's just confine this to light, wavelength, and reflection. Try looking at yourself in a full wavelength mirror. It would be somewhere between 450 and 650 nanometers wide or roughly the size of a virus or bacteria. Practicality demands a reflector vastly larger than that for simple and ordinary usage. I seriously doubt you have seen a mirror smaller than 20,000 times that size. Even so you wouldn't be able to see anything more than your eye in it - or with advanced optics, your face. Would that larger mirror have any more gain that one that was one thousandth its size? No, not to speak of in any practical sense. Texas Instruments invented the DMD for today's projection TV systems that use mirrors that small.... for one pixel of light. Their DMD chip has a vast array of at least 1000000 of these mirrors. Most of the light in the system is lost. Efficiency is thus very poor, but that is not an economic issue. In a way, it most conforms to the same issues of poor efficiency in a small radiator: most of the RF power is wasted before it gets into the sky. Unfortunately, for most practicing Hams, this is a very serious economic issue. Here's a practical challenge for the reader: Take a Christmas tree bulb of 7.5W. Employing every trick of the trade of optics, how much of that available power can you get into a 100 micron fiber optic? 73's Richard Clark, KB7QHC |
#7
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On Sep 11, 2:55*pm, Richard Clark wrote:
On Thu, 11 Sep 2008 09:38:46 -0700 (PDT), Art Unwin wrote: On Sep 11, 10:37*am, Richard Clark wrote: On Thu, 11 Sep 2008 06:18:14 -0700 (PDT), Art Unwin wrote: If I have a flash light that is focussed does this wavelength aproach still apply? The reflector (or magnifier lens, take your pick) is on order of at least 1 centimeter. *The light wavelength is on order of 500 nanometers. Ratio = 20,000:1 Beam is generally no narrower than 15 degrees. *At a distance of, say, 6 feet, that beam would cover a diameter of 18 inches. *Nothing like a Lazer (sic) if that is the goal. I see no basis for the inclusion of wavelengths when one is not using a straight radiator Read your own question. *There is no such thing as a "straight radiator" of light. *There is everything to do with wavelength or you could never see light. 73's Richard Clark, KB7QHC If you say so and are comfortable with that then stick with it ! My thoughts are with the reflector and it's design |
#8
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On Sep 11, 9:18*am, Art Unwin wrote:
On Sep 11, 2:53*am, Jon Kåre Hellan wrote: writes: Roy Lewallen wrote: wrote: Of course. Everyone knows the gain of a parabola is directly proportional to the size in wavelengths, or: G=10*log k(pi*D/L)^2 Where G= gain in DB over an isotropic, k ~ .55 for most real parabolas, D is the diameter, and L is the wavelength (wavelength and diameter in the same units. So a 2,000 foot parabola on 20m would have just about 58db gain. Hm. I get 47. Roy Lewallen, W7EL Hmm, when I use 14 Mhz and 6 decimal places I get 37; must have fat fingered it the first time. Going a different way, I also get about 37. Aperture of a dish is the area, pi*r^2. r is about 14.2 wl, so area is about 635 sq. wl. Aperture of a dipole is 1/4 * 1/2 wl = 1/8 sq. wl. That makes gain 635/(1/8) = 635*8, i.e about 5100 or just over 37 dBd. This assumes 100 % illumination of the dish, which we won't achieve. So make it 35 dBd or so, i.e. 37 dBi. Using the o.p.'s formula, I get 36.5 dBi. * It's odd that pi is squared in the formula. The squared part must be to account for the area of the dish, which is pi*r^2. Obviously, this can has been compensated for by the choice of 'k'. Whoaaa guys............! *Let us think a bit more regarding the basics presented instead of parrotting dish's as used in the present state of the art. Isn't a dish built around phase change of a half wave dipole in inter magnetic coupling? If I have a flash light that is focussed does this wavelength aproach still apply? *I thought it would be a question of action and reaction. Trow a ball against the wall and it bounces back in a reflective manner to the angle of velocity. A dish as presently used changes the phase of a given signal to reverse it's direction. In physics we can also talk about mechanical force that rebound and rebound has nothing to do with wavelength! * * *If we consider radiation as being the projection of particles instead of wavelike oscillation then surely the size of the reflector is solely based on what can be collected from the *emmitter such that it rebounds to a point or a focussed form ? *I ask the question as I know nothing about the reflective phenomina of dish's tho I have visited *the one in P.R. where the dish is formed with the knoweledge that the radiation spreads out according to the emmiter used and thus when it reaches the reflector the unit strength is weaker which the dish attempts to reverse by refocussing. But then I could be totally in error thus the question to the experts Best regards Art Unwin KB9MZ .- Hide quoted text - - Show quoted text - I think you cannot use the particle analogy with HF when dish size is not greater than wavelength. For a small dish at HF, the waves will simply bend around the dish and act as if it wasn't there. At much higher frequencies, particle concepts become more accurate. |
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