Izici
● Ukusebenza Kwebhendi Egcwele
● I-Dual Polarization
● Ukuzihlukanisa Okuphezulu
● Okwenziwe Ngokuqondile Negolide
Imininingwane
I-MT-DPHA75110-15 | ||
Into | Ukucaciswa | Amayunithi |
I-Frequency Range | 75-110 | GHz |
Inzuzo | 15 | dBi |
I-VSWR | 1.4:1 | |
I-polarization | Okukabili | |
Evundlile 3dB Beam Ububanzi | 33 | Amadigri |
Ububanzi Bebhontshisi obume 3dB | 22 | Amadigri |
Ukuhlukaniswa kwePort | 45 | dB |
Usayizi | 27.90*52.20 | mm |
Isisindo | 77 | g |
Usayizi we-Waveguide | I-WR-10 | |
Ukuqokwa kweFlange | UG-387/U-Mod | |
Body Material futhi Qeda | Ai-aluminium, igolide |
Umdwebo Wohlaka
Imiphumela Yokuhlola
I-VSWR
Umzimba oyinhloko we-antenna eplanethi iyisakhiwo se-plana yensimbi esinosayizi omkhulu kakhulu kunobude obusebenzayo.Ama-antenna e-Planar asetshenziswa ekugcineni kwefrikhwensi ephezulu ye-spectrum yomsakazo, ikakhulukazi kubhendi ye-microwave, futhi isici sawo esikhulu ukuqondisa okuqinile.Izimpondo ezijwayelekile zokuhlela zihlanganisa izimpondo zophondo, izimpondo ze-parabolic, njll., ezisetshenziswe kakhulu ezinhlelweni zokuxhumana ze-microwave relay, ukuxhumana ngesathelayithi, irada, nokuzulazula.
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