eyona nto iphambili

I-Antenna ye-Conical Dual Polarized Horn 12 dBi Type. Gain, 0.8-18GHz Frequency Range RM-CDPHA0818-12

Inkcazo emfutshane:

Imodeli ye-RF MISO i-RM-CDPHA0818-12 yi-antenna ye-lens horn ene-polarized ephindwe kabini esebenza ukusuka kwi-0.8 ukuya kwi-18GHz, I-antenna inika i-12 dBi typical gain. I-antenna i-VSWR iqhelekileyo yi-1.5:1. Ii-antenna RF ports zizixhumi ze-SMA-KFD. Ingasetyenziswa kakhulu ekufumaneni i-EMI, ukujongwa, ukuphonononga, ukulinganiswa kwe-antenna kunye neepateni kunye nezinye iindawo zesicelo.


Iinkcukacha zeMveliso

Ulwazi lwe-Antenna

Iithegi zeMveliso

Iimbonakalo

● I-Coaxial Adapter yee-RF Inputs

● I-Antena yelensi

● Ukusebenza kweBroadband

● I-VSWR ephantsi

Iinkcukacha

RM-CDPHA0818-12

Iiparameters

Okuqhelekileyo

Iiyunithi

Uluhlu lweeFrequency

0.8-18

I-GHz

Inzuzo

Uhlobo lwe-12.

dBi

I-VSWR

1.5 Uhlobo.

 

Ukwahlulahlula

Isibini Imigca ethe tyaba

 

Ukuzahlula kwi-Cross Pol.

25

dB

Ukuzahlula kwiZibuko

30

dB

 Isinxibelelanisi

I-SMA-KFD

 

Izinto eziphathekayo

Al

 

Ukugqiba

PaintMnyama

 

Ubungakanani

295*Ф198(L*W*H)

mm

Ubunzima

2.6

kg

Ulawulo lwaMandla, CW

50

W

Ukuphatha Amandla, Incochoyi

100

W


  • 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