Imodyuli ye-RF Amplifier ye-Mars RF's Wideband MM00210P49A
Intshayelelo yemveliso
Le sixhobo sokukhulisa i-rf esibanzi esivela kwiMars RF sinikezela ngoluhlu olubanzi lwe-dynamic, amandla aqhelekileyo okugcwala kwe-RF angama-80 watts, kunye nokwanda kwamandla e-RF angama-49 dB. Sisebenza phakathi kwe-20 MHz kunye ne-1000 MHz. Le sixhobo sokukhulisa i-rf esibanzi senzelwe usetyenziso lwe-P-band olufana ne-jamming, i-EMC, kunye novavanyo kunye nokulinganisa. Iqela loyilo kwiMars RF alipheli ekufuneni ukugqwesa, liqinisekisa ukuba imveliso nganye eyenziwe yiMars RF ihlangabezana nemigangatho ephezulu. Emva kokuvavanywa ngokungqongqo, isixhobo sokukhulisa i-rf esibanzi sinemilinganiselo yokusebenza emangalisayo. Ngokukodwa, ii-harmonics zale sixhobo sokukhulisa i-rf esibanzi zihlala ziyi--10dBc, nto leyo ebonisa ukuphambuka okuncinci kwe-harmonic kunye nokukhupha isignali ecocekileyo. Ngaphezu koko, isignali engeyiyo idla ngokuba yi--55dBc, nto leyo eqinisekisa ukuba kukho ukuphazamiseka okuphantsi kwezinye iinkqubo.
Umlinganiselo wamaza okuma we-wideband rf amplifier (SWR) zizinto ezibalulekileyo ezibonisa indlela i-amplifier kunye nomthwalo wayo ohambelana ngayo ne-impedance. Umlinganiselo wamaza okuma (SWR) wesi sixhobo se-wideband rf amplifier esivela kwi-Mars RF unokufikelela kwi-3:1, nto leyo ekhokelela ekusebenzeni ngcono nasekuthembekeni. Esi sixhobo se-solid state power amplifier (SSPA) sisebenza kakuhle kakhulu, sifikelela kwi-30%, xa amandla okukhupha i-RF eyi-30Watts. Isixhumi se-DC interface yi-D-Sub 9-Pin, Male.
Iiparameters
| Qalisa i-frequency | 20 MHz |
| Isantya sokumisa | 1000 MHz |
| Imveliso yeRF | IiWatts ezingama-80 eziqhelekileyo |
| Ukwanda kwamandla e-RF | I-49 dB eqhelekileyo |
| I-voltage yokusebenza | I-28V eqhelekileyo |
| Ukusebenza kakuhle @80W | 30% |
Ezona mpawu
√ Isandisi-lizwi se-RF se-Class AB wideband
√ Usetyenziso lwebhendi ye-P
√ Uluhlu lweefrikhwensi: 20 MHz ukuya kwi-1000 MHz
√ Ukusebenza kakuhle kakhulu: 30%
√ Uyilo oluncinci
√ I-VSWR: 3:1

Ubuchule bokuhlanganisana okuncinci
I-Mars RF iseke iClass100,000 "Amagumbi acocekileyo" eworkshop yokucoca i-micro-assembly ukuqinisekisa ukusebenza okuphezulu kwayo yonke imveliso yethu ye-wideband rf amplifier. Ukuze sibonelele ngendawo efanelekileyo yokuvelisa iimveliso ze-micro-assembly, sisebenzisa izixhobo zokucoca umoya ezisemgangathweni ophezulu kunye nemigangatho yococeko engqongqo kule workshop yokuvelisa yobuchwepheshe obuphezulu ukuze sihluze kwaye sisuse amasuntswana amancinci emoyeni ngokufanelekileyo. Kwaye sinesebe lethu le-micro-assembly, elisivumela ukuba silawule umgangatho wemveliso ngokwethu kwaye senze ukusebenza kwezi amplifier ezinamandla aphezulu kunye namandla aphezulu kuhambelane ngakumbi.
FAQ
1. Ngaba ungenza ngokwezifiso umsebenzi wokukhusela amaza amiyo kwiimveliso zakho ze-wideband rf amplifier?
Abathengi banokwazisa iqela lethu ngeemfuno zabo kwaye siya kuxhasa iinkonzo zokwenza ngokwezifiso imveliso ukuba baneemfuno ezithile zeenkcukacha zemveliso ye-wideband rf amplifier okanye uvavanyo kunye nokuhlolwa okunxulumene noko. Ke ngoko, uphawu lokukhusela amaza amileyo lunokwenziwa ngokwezifiso ukuhlangabezana neemfuno zomthengi. Olu phawu lujoliswe ekukhuseleni umonakalo wamaza amileyo kwimodyuli ye-power amplifier okanye kwinkqubo engaphantsi.



LEYA
Iradar
Uvavanyo kunye noLinganiselo
Unxibelelwano