I-Dual Circular polarization probe 10dBi Typ.Gain, 17-22GHz Frequency Range RM-DCWPA1722-10

Incazelo emfushane:

Imininingwane Yomkhiqizo

UNYAZI LWE-ANTENNA

Omaka bomkhiqizo

Imininingwane

RM-I-DCWPA1722-10
Into	Ukucaciswa	Amayunithi
I-Frequency Range	17-22	GHz
Zuza	10Thayipha.	dBi
I-VSWR	<1.3
I-polarization	Indilinga Ekabili
I-Cross Polarization	40 Uhlobo.	dB
Ukuhlukaniswa kwePort	27 Uhlobo.	dB
AR	<0.75	dB
Indiza ye-3dB Beamidth-E	61 Uhlobo.	°
Indiza ye-3dB Beamidth-H	61 Uhlobo.	°
Isixhumi	I-SMA-F
Usayizi(LWH)	121.693.630.8	mm
Isisindo	0.058	Kg
Body Material	Al
Ukuphatha Amandla, CW	50	W
Ukuphatha Amandla, Peak	3000	W

Okwedlule: I-Standard Gain Horn Antenna 25dBi Typ. Thola, 50-75 GHz Frequency Range RM-SGHA15-25

Olandelayo: I-Dual Circular polarization probe 10dBi Typ.Gain, 27-31GHz Frequency Range RM-DCWPA2731-10

I-Dual Circular Polarized Horn Antenna iyingxenye ye-microwave eyinkimbinkimbi ekwazi ukudlulisa kanye/noma ngesikhathi esisodwa amagagasi aPolarized Polarized Asesandleni sobunxele nakwesokudla. Le antenna ethuthukisiwe ihlanganisa i-polarizer eyisiyingi ne-Orthogonal Mode Transducer ngaphakathi kwesakhiwo sezimpondo eziklanywe ngokunembile, evumela ukusebenza okuzimele eziteshini ezimbili eziyindilinga zokuhlukanisa phakathi kwamabhendi abanzi.

Izici Zobuchwepheshe Ezibalulekile:

Ukusebenza kwe-CP ekabili: Izimbobo ezizimele ze-RHCP ne-LHCP
I-Low Axial Ratio: Ngokuvamile i-<3 dB yonkana ibhendi yokusebenza
Ukuhlukaniswa Kwembobo Ephakeme: Ngokuvamile >30 dB phakathi kwamashaneli e-CP
Ukusebenza kwe-Wideband: Ngokuvamile ngu-1.5:1 kuya ku-2:1 isilinganiso sefrikhwensi
Isikhungo Sesigaba Esizinzile: Ibalulekile ekusetshenzisweni kokulinganisa ukunemba

Izinhlelo zokusebenza eziyinhloko:

Amasistimu okuxhumana ngesathelayithi
I-radar ye-polarimetric nokuzwa okukude
I-GNSS nezinhlelo zokusebenza zokuzulazula
Ukulinganisa nokulinganisa kwe-antenna
Ucwaningo lwesayensi oludinga ukuhlaziywa kwe-polarization

Lo mklamo we-antenna unciphisa ngempumelelo ukulahlekelwa kwe-polarization okungafani kahle kuzixhumanisi zesathelayithi futhi uhlinzeka ngokusebenza okuthembekile ezinhlelweni zokusebenza lapho i-polarization yesignali ingase ihluke ngenxa yezinto zemvelo noma umumo weplathifomu.