| SatSig Topics Index › Dish pointing and alignment › Dish replacement |
SatSig topic: Dish replacement(Read 9440 times) |
|
Dec 20th, 2012 at 1:26am
Thanks. |
|
Dec 21st, 2012 at 12:23am
//greg// |
|
Dec 21st, 2012 at 6:13am
|
|
Dec 21st, 2012 at 12:12pm
Now that's just theory, with a little technical jargon sprinkled in. Actually finding one will not only be difficult, it will be expensive. The most common consumer mesh reflectors are for C-band use, the smallest of which is typically a 10 foot diameter. But assuming I'm correct that portability is more important to you than mesh, you should have better luck searching for a smaller high gain solid dish. Try ViaSat, General Dynamics, Global TT. And another good search phrase to use would be "fly-away internet". Here's an example: https://www.mobilsat.com/Flyaway-transportable-satellite-internet/ //greg// |
|
Dec 21st, 2012 at 2:25pm
4 GHz (C band receive only, e.g. TV) wavelength = 300/4 = 75 mm Surface tolerance = 9.4 mm 11 GHz (C band receive only, e.g. TV) wavelength = 300/11 = 27 mm Surface tolerance = 3.5 mm The surface accuracy of a dish, for transmit gain and sidelobe quality, should be about 1/10th wavelength or better. 4/6 GHz (C band VSAT tx/rx) wavelength at 6 GHz = 300/6 = 50 mm Surface tolerance = 5 mm 11/14 GHz (Ku band VSAT tx/rx) wavelength at 14 GHz = 300/14 = 21 mm Surface tolerance = 2 mm 20/30 GHz (Ka band VSAT tx/rx) wavelength at 30 GHz = 300/30 = 10 mm Surface tolerance = 1 mm If you have a distorted dish, the gain can be much lower (e.g. 4.5 dB low) compared with what you expected. Sidelobe performance will be appalling and you will cause unacceptable interference into services on nearby satellites. Open wire mesh dishes will work at C band for receive only TV. At Ku band you need a perforated metal sheet. At Ka band you need a solid metal surface. 'Plastic' dishes have a fine wire mesh just beneath the surface or a metalised film layer under the front surface. 'Plastic' dishes with wire mesh hidden inside may only work acceptably at C band. The feed horn, the feed support arm and the dish are designed as a whole and all three parts should be kept together. The feedhorn has a radiation pattern of its own and 'illuminates' the main reflector surface. The illumination pattern is important to obtain the best compromise of both good enough on-axis gain and good enough off-axis sidelobe performance. The feed must aim accurately at the dish so that the edge illumination, typically -16 dB down, is the same all around, otherwise sidelobes start coming up. The system needs to be in focus with the feed phase centre at the focal point of the dish. Rely strictly on use of the manufacturers feed support arm and assembly instructions. At Ku band, a number of manufacturers make easy-to-carry 'flight-case' antennas, in segments that clip together. These are high precision products with accurately aligning clips. They are often made of carbon fibre and are very expensive. Best regards, Eric. |
|
Dec 26th, 2012 at 8:38am
I thought I'd note that Eric's mention of 1/8 to 1/10 lambda means surface tolerance RMS, so all the reflector surface roughness adds up and produces noise. This means that if you are going to actively transmit to space, just using any dish that matches the gain is not going to be enough. You also need an accurate reflector shape. If you are producing too much noise then the satellite operator will ask to shut down your terminal in order to avoid service degradation for other customers. The same thing may happen if your feed has a different focal point/radiation pattern than the reflector was designed for. The best option is indeed to go with a fly away antenna from a reputable vendor. It's expensive, but it's the only way you can be sure you are not going to cause troubles on the satellite, unless you want to build your own full blown lab to test your antenna (and probably certify it with the satellite operator as it may be required.) |
|
Email me:eric@satsig.net |