eyona nto iphambili

I-Antenna ye-Cassegrain 26.5-40GHz Uluhlu lokuphindaphinda, ukufumana i-40dBi Typ.RM-CGA28-40

Inkcazo emfutshane:


Iinkcukacha zeMveliso

ULWAZI LWEE-ANTEN

Iithegi zeMveliso

Iinkcukacha

RM-CGA28-40

Iiparameters

Inkcazo

Iyunithi

Uluhlu lweeFrequency

26.5-40

I-GHz

Isikhokelo samaza

WR28

Inzuzo

40 Uhlobo.

i-dBi

I-VSWR

1.2 Uhlobo.

Ukwahlulahlula

 Imigca ethe tyaba

  Ujongano

Isikhokelo seWave /2.92-Ibhinqa

Izinto eziphathekayo

Al

Ukugqiba

Paint

Ubungakanani

Φ625.0*434.9(±5)

mm

Ubunzima

9.088

kg


  • Ngaphambili:
  • Okulandelayo:

  • I-antenna yeCassegrain yi-antenna esebenza kakuhle kakhulu ene-dual-reflector, egama layo kunye noyilo lwayo luvela kwi-telescope yeCassegrain. Iqulathe i-reflector ephambili (i-paraboloid) kunye ne-reflector yesibini (i-hyperboloid), ebekwe ngaphezulu kwendawo ephambili ye-reflector ephambili.

    Umgaqo wayo wokusebenza ngolu hlobo lulandelayo: uphondo lokutya luqala ngokusasaza amaza e-electromagnetic ukuya kwi-reflector yesibini, ethi emva koko ibonise amaza kwi-reflector ephambili. I-reflector ephambili idibanisa la maza ibe ngumqadi ohambelanayo, ojolise kakhulu ekudluliseleni. Le ndlela "egobileyo" ye-optical ivumela i-feed ukuba ifakwe ngasemva kwe-reflector ephambili, nto leyo enciphisa kakhulu ilahleko ye-feedline kwaye yenza kube lula ukugcinwa.

    Iingenelo eziphambili zale antenna kukufumana kwayo okuphezulu, ii-lobes ezisecaleni ezisezantsi, isakhiwo esincinci (xa kuthelekiswa neparabola ende), kunye nokubekwa kwe-feed kunye nee-receiver ngasemva kwe-reflector ephambili, nto leyo enciphisa ukulahleka kothumelo. Ingxaki yayo ephambili kukuvaleka kwenxalenye ye-main beam yi-reflector yesibini kunye nesakhiwo sayo sokuxhasa. Isetyenziswa kakhulu kunxibelelwano lwesathelayithi, i-radio astronomy, kunye neenkqubo ze-radar ezikude.

     
     
     

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