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

I-Antenna yeCassegrain 26.5-40GHz iFrequency Range, Gain 40dBi Typ.RM-CGA28-40 Featured Image

Inkcazo emfutshane:

Qhagamshelana nathi Fumana iSheet yeDatha yeMveliso

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: I-Antenna yePolarized Horn ejikelezileyo ephindwe kabini eyi-15dBi Uhlobo lokufumana, 18-26.5 GHz Ububanzi beFrequency RM-DCPHA1826-15

Okulandelayo: I-RHCP Log Spiral Antenna 3.5dBi Uhlobo lokufumana, 0.1-1 GHz Ububanzi boHlala lweRhafu RM-LSA011-4R

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.