Ukugxila Komkhiqizo
I-RM-DCGHA1822-20 I-Dual Linear Polarization Corrugated Horn Antenna
Konjiniyela be-RF abasebenza ebhendini le-18-22 GHz, ukuzinza kwe-antenna kungaphezu kwencazelo eshidini ledatha. I-antenna yokuhlola idinga inzuzo ebikezelwayo, ukuziphatha okulawulwayo kwe-polarization, kanye nokuhambisana okuthembekile kwe-impedance kulo lonke ibhendi yokusebenza. I-RF MISORM-DCGHA1822-20kuyintoi-antenna yophondo oluhlanganisiwe olunemigqa emibilieyenzelwe ukulinganisa i-microwave, ukuhlolwa kwe-radar, ukuhlolwa kwesistimu yokuxhumana, kanye nokuhlanganiswa kwe-RF ezwela ukuhlukaniswa kwe-polarization.
Lo modeli usebenza kusukela18 kuya ku-22 GHzfuthi inikezaInzuzo yohlobo lwe-dBi engu-20ngeUhlobo lwe-VSWR 1.5:1.Isakhiwo sempondo egobile sisekela izici zokukhanya okuhlanzekile kanye nokuziphatha kokukhanya okuzinzile, okwenza i-antenna ifanelekele izindawo zobunjiniyela lapho ukuphindaphindeka nokusebenza kokuqondisa kubalulekile khona.ukuhlukaniswa okuqondile okubili, abasebenzisi bangasebenza neziteshi ezimbili ze-orthogonal linear polarization emzimbeni owodwa we-antenna, okunciphisa isidingo sokushintsha ama-antenna ngokomzimba ngesikhathi sokuqhathaniswa kwe-polarization noma ukuqinisekiswa kwesistimu.
Ngokusho kweshidi ledatha le-RF MISO, i-RM-DCGHA1822-20 inikezaUkwehlukaniswa kwe-cross polarisation okungu-35 dBUkuze kusethwe ukuhlolwa okusebenzayo, lokhu kusiza onjiniyela ukuthi bahlole ukuhlukaniswa kwe-polarization, ukuqondanisa i-antenna, kanye nokuziphatha kwesiteshi ezindaweni ezilawulwayo ze-RF. I-antenna isebenzisa i-Isixhumi sesifazane esingu-2.92 mm, umzimba we-aluminium onesiphetho esipendiwe, usayizi omncane womshini129.3 x Ø 72.1 mm, kanye nesisindo0.166 kg.
Imininingwane Eyinhloko
| Imodeli | RM-DCGHA1822-20 |
| Ibanga Lokuvama | 18-22 GHz |
| Inzuzo | Uhlobo lwe-20 dBi. |
| I-VSWR | Uhlobo lwe-1.5:1. |
| Ukwehlukaniswa | Umugqa Okabili |
| Ukuhlukaniswa Kwesiphambano | Uhlobo lwe-35 dB. |
| Ububanzi be-3 dB, Imbobo 1 | I-E-Plane: 18.3-22.4 deg; I-H-Plane: 17.7-21.2 deg |
| Ububanzi be-3 dB, Imbobo 2 | I-E-Plane: 18.3-22.4 deg; I-H-Plane: 17.8-21.2 deg |
| Isixhumi | Owesifazane ongu-2.92 mm |
| Izinto / Ukuqeda | I-aluminium, isiphetho esipendiwe |
| Usayizi / Isisindo | 129.3 x Ø 72.1 mm; 0.166 kg |
Izicelo Ezijwayelekile
I-RM-DCGHA1822-20 ifaneleka ekulinganisweni kwe-antenna, ukuqhathanisa ilabhorethri ye-RF, ukuhlolwa kwe-radar kanye nokuzwa, ukuhlolwa kwezixhumanisi zokuxhumana nge-microwave, ukuhlolwa kokwehlukahlukana kwe-polarization, kanye nokuhlanganiswa kwezinga lesistimu kububanzi be-18-22 GHz. Inhlanganisela yayo ye-dual linear polarization, i-standard 20 dBi gain, kanye nokwakhiwa kwe-compact corrugated horn kwenza kube ukukhetha okusebenzayo konjiniyela abadinga i-antenna ethembekile yokuhlola i-microwave okuphindaphindwayo.
Amanothi Okukhetha Onjiniyela
Uma ukhetha i-antenna yophondo olugobile, onjiniyela kufanele bacabangele ukumbozwa kwemvamisa okudingekayo, izinga lokuzuza, imodi yokwehlukanisa, isikhombimsebenzisi sokuxhuma, isikhala sokufaka ngomshini, kanye nendawo yokulinganisa. Kumasethingi okuhlola aphindwe kabili, kubalulekile futhi ukubuyekeza ukuhlukaniswa kwe-cross polarization, i-beamwidth, kanye nokucushwa kwe-port ngaphambi kokuhlanganiswa kokugcina. Uma i-antenna izosetshenziswa ekamelweni, endaweni yokulinganisa, noma njengengxenye yendlela yokulinganisa ephindaphindwayo, i-RF MISO ingasiza ekubuyekezeni imininingwane ye-antenna kanye nezidingo zesistimu yekhasimende.
Kungani Ukhethe i-RF MISO
I-RF MISO ithuthukisa futhi ikhiqize ama-antenna namadivayisi okuxhumana ezinhlelo zokusebenza zezentengiselwano, zokuhlola, kanye nezinhlelo zokuhlola. Kulo modeli, ithimba lethu lingasekela amakhasimende ngokukhetha umkhiqizo, izidingo zokuxhuma, ukufanisa uhlelo lokusebenza, kanye nemibhalo yobuchwepheshe ngaphambi kokuthenga.
Udinga i-antenna yophondo oluphindwe kabili engu-18-22 GHz?
Buyekeza ikhasi lomkhiqizo le-RM-DCGHA1822-20 noma uxhumane ne-RF MISO ukuthola ukwesekwa kobuchwepheshe kanye nemininingwane yekhotheshini.
Isikhathi sokuthunyelwe: Septhemba-04-2026

