Isihlukanisi Samandla Sezindlela Ezingu-32, 2~18GHz, 30W, SMA

Isihlukanisi samandla se-RF esinezindlela ezingu-32 siyidivayisi engenzi lutho esabalalisa ngokulinganayo isignali eyodwa ye-RF kumasignali okukhipha angu-32. Izici zayo kanye nezinhlelo zokusebenza zimi kanje:

Izici
1. Amandla okwabelana ngamandla aphezulu: ayakwazi ukusabalalisa ngokulinganayo izimpawu ze-RF zokufaka kuma-port okukhipha angu-32, adinga amandla aphezulu ukuze abhekane nezimo zokufaka ezinamandla aphezulu njengeziteshi zesisekelo noma izinhlelo ze-radar.
2. Ukuhlukaniswa okuphezulu: Imbobo ngayinye yokuphuma inezinga eliphezulu lokuhlukaniswa ukuze kugwenywe ukuphazamiseka okuhlangene phakathi kwezimpawu.
3. Izici ze-Broadband: Ububanzi bokumbozwa kwemvamisa ebanzi, kusukela ku-direct current (DC) kuya kuma-microwave frequency aphezulu, njengo-40GHz noma ngaphezulu.
4. Ukufaniswa okuhle kwe-impedance: Kunganikeza ukufaniswa okuhle kwe-impedance engu-50 Ω, kunciphise ukubonakaliswa kwesignali, futhi kuthuthukise ukusebenza kahle kokudlulisa.
5. Amandla aphezulu: Ezinye izihlukanisi zamandla ze-RF ezinezindlela ezingu-32 zingamelana namandla aphezulu futhi zifanele ukusetshenziswa kwamandla aphezulu.
6. Ukuvumelana kwesigaba kanye ne-amplitude: Isigaba sesignali kanye ne-amplitude ye-output port ngayinye kuhle, kufanelekile ezinhlelweni zokusebenza ezidinga ikhwalithi ephezulu yesignali.

Isicelo
1. Uhlelo lokuxhumana: Lungasetshenziswa ukusabalalisa amasignali kuma-antenna amaningi, ukufeza imisebenzi yokubekezelela inzuzo namaphutha kwezinhlelo zama-antenna amaningi, nokuthuthukisa ukumbozwa kokuxhumana kanye nokuthembeka.
2. I-radar kanye ne-electronic warfare: yabela amasignali amakhulu noma izinkulungwane zamayunithi e-antenna, isekela ukwakheka kwe-beamforming kanye nokuskena okusheshayo; Ukukhiqizwa kanye nokusatshalaliswa kwamasignali okuphazamiseka kweziteshi eziningi.
3. Imishini yokuhlola: Amadivayisi amaningi ahlolwayo (i-DUT) asebenza ngasikhathi sinye emishinini yokuhlola eneziteshi eziningi ukuthuthukisa ukusebenza kahle kokuhlola, njengokuhlolwa kwe-RF chip noma i-antenna array.
4. Ucwaningo lwelabhorethri: Ucwaningo olukhulu lwe-MIMO, ukuhlolwa kokuvumelanisa kwe-quantum multi-channel, noma ukucubungula amasignali e-array ku-radio astronomy.

Isihlukanisi samandla se-RF esinezindlela ezingu-32, esinekhono laso lokusabalalisa iziteshi eziningi, sisetshenziswa kabanzi ezimweni zokucubungula amasignali aphezulu. Kodwa-ke, ukwakheka nokukhiqiza kwaso kudinga ukulinganisela ukulahlekelwa, ukuhlukaniswa, ivolumu, kanye nezindleko, okudala izinselele ezinkulu zobuchwepheshe.