I-Antenna ye-Planar Spiral 5 dBi Typ. Ukuzuza, 18-40 GHz Frequency Range RM-PSA1840-5

I-Antenna ye-Planar Spiral 5 dBi Typ. Gain, 18-40 GHz Frequency Range RM-PSA1840-5 Umfanekiso ofakiweyo

Inkcazelo emfutshane:

Imodeli ye-RF MISO ye-RM-PSA1840-5 yi-eriyali yesandla sasekunene ejikelezayo ejikelezayo esebenza ukusuka kwi-18 ukuya kwi-40GHz. Yenzelwe i-EMC, ukuqwalaselwa kwakhona, ukuqhelaniswa, ukuvalelwa kude, kunye nosetyenziso lwezithuthi ezigungxulwayo. Ezi-eriyali ze-eriyali zinokusetyenziswa njengamacandelo e-eriyali ahlukeneyo okanye njengezondla ii-eriyali ezibonisa i-eriyali.

Qhagamshelana nathi Fumana iDatha yeMveliso

Iinkcukacha zeMveliso

Ulwazi lwe-antenna

Iithegi zeMveliso

Iimbonakalo

● Ilungele ukusetyenziswa emoyeni okanye emhlabeni

● I-VSWR ephantsi

● I-RH Circular Polarization

● NgeRadome

Iinkcukacha

RM-PSA1840-5
Iiparamitha	Isiqhelo	Iiyunithi
Uluhlu lokuphindaphinda	18-40	GHz
Inzuzo	5 Isimbo.	dBi
VSWR	≤2.5 Isimbo.
Ipolarization	RH Setyhula Polarization
Isidibanisi	2.92-Owasetyhini
Izinto eziphathekayo	Al/Epoxy fiberglass
3dB ububanzi beBeam	60°- 80°
Ubungakanani(LWH)	Φ33.2*36.9(±5）	mm
I-Antenna Cover	Ewe
Into evikela amanzi	Ewe
Ubunzima	0.01	Kg
Ukuphathwa kwamandla, CW	1	w
Ukuphathwa kwamandla, iPeak	50	w

Ngaphambili: Iprobe ye-polarization yeSetyhula ephindwe kabini 10dBi Typ.Gain, 27-31GHz Frequency Range RM-DCWPA2731-10

Okulandelayo: I-Antenna ye-Broadband Horn 10 dBi Typ.Gain, 0.8 GHz-8 GHz Frequency Range RM-BDHA088-10

I-eriyali ecetyiweyo yi-eriyali yakudala ezimeleyo eyaziwayo ngeempawu zayo ze-ultra-wideband. Ubume bayo buqulathe iingalo zentsimbi ezimbini nangaphezulu ezijikela ngaphandle ukusuka kwindawo yesondlo esembindini, kunye neentlobo eziqhelekileyo yiArchimedean spiral kunye nelogarithmic spiral.

Ukusebenza kwayo kuxhomekeke kwisakhiwo sayo sokuzixhasa (apho isinyithi kunye nezithuba zomoya zinemilo efanayo) kunye nengcamango "yengingqi esebenzayo". Kwi-frequency ethile, ummandla ofana nesangqa kungqukuva onesangqa esimalunga ne-wavelength enye uyachulumanca kwaye ube ngummandla osebenzayo onoxanduva lokusasazeka kwemitha. Njengoko i-frequency itshintsha, lo mmandla usebenzayo uhamba ngeengalo ezijikelezayo, nto leyo ivumela iimpawu zombane ze-eriyali ukuba zihlale zizinzile kwi-bandwidth ebanzi kakhulu.

Iinzuzo eziphambili zale eriyali yi-bandwidth yayo ye-ultra-wide (idla ngokuba yi-10: 1 okanye ngaphezulu), amandla endalo kwi-polarization yesetyhula, kunye neepateni ezizinzileyo zemitha. Iintsilelo zayo eziphambili bubungakanani bayo obukhulu kwaye ngokuqhelekileyo inzuzo ephantsi. Isetyenziswa kakhulu kwizicelo ezifuna ukusebenza kwe-ultra-wideband, njengemfazwe yombane, unxibelelwano lwebroadband, imilinganiselo ye-time-domain, kunye neenkqubo zeradar.