Iinkcukacha
| RM-CKHA75-20 | ||
| Iiparamitha | Inkcazo | Iyunithi |
| Uluhlu lokuphindaphinda | 10-15 | GHz |
| Inzuzo | 20 Isimbo. | dBi |
| VSWR | <1.3 |
|
| Ipolarization | I-LHCP |
|
| I-Cross Polarization | 30 Chwetheza. | dB |
| AR | <2 | dB |
| 3dB Beamwidth,E-Plane | 12.9-19.8 | deg |
| 3dB Beamwidth,H-Plane | 12.7-19.7 | deg |
| Isidibanisi | I-SMA-Ibhinqa |
|
| Umkhombandlela wamaza | I-WR75 |
|
| Izinto eziphathekayo | Al |
|
| Ukugqiba | Phayi |
|
| Ubungakanani(L*W*H) | 498.2 * 140.4 * 147.0 | mm |
| Ubunzima | 1.35 | Kg |
I-Antenna ye-Corrugated Horn yi-eriyali ye-microwave ekhethekileyo enezinto ezityalwa ngamaxesha athile (imijelo) ecaleni komphezulu wodonga lwayo olungaphakathi. Ezi corrugations zisebenza njengezinto ezihambelana nomphezulu we-impedance, zicinezela ngokufanelekileyo imisinga yomphezulu onqamlezayo kunye nokwenza ukuba ukusebenza kombane okhethekileyo.
Iimpawu eziphambili zobuGcisa:
-
I-Ultra-Low Sidelobes: Ngokuqhelekileyo ngaphantsi kwe-30 dB ngokusebenzisa ulawulo lwangoku lwangoku
-
Ucoceko oluphezulu lwePolarization: Ucalucalulo lwe-cross-polarization lungcono kune -40 dB
-
Ipateni ye-Symmetrical Radiation: Iphantse ifane i-E- kunye ne-H-plane iipateni zomqadi
-
Iziko leSigaba esiZinzile: Ukwahluka kweziko lesigaba esincinci kwibhendi yamaza
-
Ubungakanani bobubanzi obubanzi: Ngokuqhelekileyo isebenza kwi-1.5: i-1 frequency ratios
Usetyenziso Olungundoqo:
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Iinkqubo zokutya konxibelelwano lwesathelayithi
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Iiteleskopu zeRadio astronomy kunye nabamkeli
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Iinkqubo ze-metrology ezichanekileyo
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I-Microwave imaging kunye ne-remote sensor
-
Iinkqubo ze-radar ezisebenza kakhulu
Ulwakhiwo olubiyelweyo luvumela le eriyali ukuba ifezekise iimpawu zokusebenza ezingenakufikelelwa ziimpondo eziqhelekileyo zodonga olugudileyo, ngakumbi kwizicelo ezifuna ulawulo oluchanekileyo lwangaphambili kunye nemitha eyinkohliso encinci.
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