engundoqo

I-Antenna ye-Corrugated Horn 22dBi Typ Gain, 140-220GHz Frequency Range RM-CGHA5-22

Inkcazelo emfutshane:


Iinkcukacha zeMveliso

ULWAZI LWE-ANTENNA

Iithegi zeMveliso

Iinkcukacha

RM-CGHA5-22

Iiparamitha

Inkcazo

Iyunithi

Uluhlu lokuphindaphinda

140-220

GHz

Inzuzo

22 Chwetheza. 

dBi

VSWR

1.6 Isimbo

 

Ukubekwa wedwa

30 Chwetheza.

dB

Ipolarization

Umgca

 

Umkhombandlela wamaza

I-WR5

 

Izinto eziphathekayo

Al

 

Ukugqiba

Phayi

 

Ubungakanani(L*W*H)

30.4*19.1*19.1 (±5)

mm

Ubunzima

0.011

kg


  • Ngaphambili:
  • Okulandelayo:

  • 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:

    1. Iinkqubo zokutya konxibelelwano lwesathelayithi

    2. Iiteleskopu zeRadio astronomy kunye nabamkeli

    3. Iinkqubo ze-metrology ezichanekileyo

    4. I-Microwave imaging kunye ne-remote sensor

    5. 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.

    Fumana iDatha yeMveliso