eyona nto iphambili

I-Antenna ye-Conical Dual Polarized Horn 18 dBi Type. Gain, 42-44GHz Frequency Range RM-CDPHA4244-18

Inkcazo emfutshane:

Imodeli ye-RF MISO i-RM-CDPHA4244-18 yi-antenna ene-polarized horn ephindwe kabini esebenza ukusuka kwi-42 ukuya kwi-44GHz, I-antenna inika i-18 dBi typical gain. I-antenna i-VSWR iqhelekileyo yi-1.5:1. Ii-antenna ze-RF ports ziyi-2.4-KFD Female connector. Ingasetyenziswa kakhulu ekufumaneni i-EMI, ukujongwa, ukuhlaziya, ukulinganisa i-antenna gain kunye nepateni kunye nezinye iindawo zesicelo.


Iinkcukacha zeMveliso

Ulwazi lwe-Antenna

Iithegi zeMveliso

Iimbonakalo

● I-Coaxial Adapter yee-RF Inputs

● Inzuzo Ephezulu

● I-Dual Linear Polarized

● Ubungakanani obuncinci

Iinkcukacha

RM-CDPHA4244-18

Iiparameters

Okuqhelekileyo

Iiyunithi

Uluhlu lweeFrequency

42-44

I-GHz

Inzuzo

Uhlobo lwe-18. 

dBi

I-VSWR

1.5 Uhlobo.

 

Ukwahlulahlula

Isibini Imigca ethe tyaba

 

Ukuzahlula kwiZibuko

30

dB

Ukulahleka kokucamngca

15

dB

 Isinxibelelanisi

2.4-KFD

 

Izinto eziphathekayo

Cu

 

Ukugqiba

I-Glod Plasted

 

Ubungakanani

66.5*34.8*34.8(L*W*H)

mm

Ubunzima

0.0042

kg


  • Ngaphambili:
  • Okulandelayo:

  • I-Antenna yeConical Dual Polarized Horn imele uphuhliso oluntsonkothileyo kuyilo lwe-antenna ye-microwave, idibanisa ulungelelwaniso oluphezulu lwe-geometry ye-conical kunye nokukwazi kwe-dual-polarization. Le antenna inesakhiwo se-conical flare esithambileyo esivumela iitshaneli ezimbini ze-orthogonal polarization, ezihlala zidityaniswa nge-advanced Orthogonal Mode Transducer (OMT).

    Iingenelo eziphambili zobugcisa:

    • Ulungelelwaniso oluKhethekileyo lwePateni: Igcina iipatheni zemitha ezilinganayo kuzo zombini iiplani ze-E kunye ne-H

    • Iziko leSigaba esiZinzileyo: Libonelela ngeempawu zesigaba ezihambelanayo kwi-bandwidth yokusebenza

    • Ukuhlukaniswa kweePort eziPhakamileyo: Ngokwesiqhelo kudlula i-30 dB phakathi kweetshaneli ze-polarization

    • Ukusebenza kweWideband: Ngokubanzi kufikelela kumlinganiselo wefrikhwensi ye-2:1 okanye ngaphezulu (umz., 1-18 GHz)

    • Ukuphola okuPhantsi kwe-Cross-Polarization: Ngokwesiqhelo kungcono kune -25 dB

    Izicelo eziphambili:

    1. Iinkqubo zokulinganisa ii-antenna ezichanekileyo kunye nokulinganisa

    2. Izixhobo zokulinganisa i-radar cross-section

    3. Uvavanyo lwe-EMC/EMI olufuna ukwahluka kwe-polarisation

    4. Izikhululo zomhlaba zonxibelelwano lwesathelayithi

    5. Uphando lwezenzululwazi kunye nokusetyenziswa kwe-metrology

    Ijiyometri yekhoni inciphisa kakhulu iziphumo ze-edge diffraction xa kuthelekiswa noyilo lwe-pyramidal, nto leyo ebangela iipateni zemitha ezicocekileyo kunye nokukwazi ukulinganisa ngokuchanekileyo. Oku kuyenza ibe luncedo kakhulu kwizicelo ezifuna ubumsulwa obuphezulu beepateni kunye nokuchaneka kokulinganisa.

    Fumana iSheet yeDatha yeMveliso