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Ukuthembeka okuphezulu kunye nokuqina kwe-Wideband RF Amplifier MM0527P43B

Inombolo yoMzekelo: MM0527P43B

I-amplifier ye-rf ye-wideband ye-Mars RF i-MM0527P43B isebenza phakathi kwe-500 - 2700MHz kunye nokunyuka kwe-43dB. Inika uluhlu lwesignali ye-RF enamandla aqhelekileyo angama-20 Watts agcweleyo. Le amplifier ye-rf ye-wideband yenziwe ngehardware ye-RF ekumgangatho ophezulu kunye nenkqubo yovavanyo lwe-amplifier ephucukileyo, enokuphucula ukusebenza kwee-amplifier ze-rf ze-wideband ngokubanzi.

  • Qala 500 MHz
  • Yeka 2700 MHz
  • I-Pout Iiwatts ezingama-20
  • Inzuzo 43 dB
  • I-Voltage 28 V
  • Okwangoku 4 Amp
  • Imo I-CW
  • Ubungakanani 140x85x25 mm

Intshayelelo yemveliso

Imodeli iMM0527P43B yi-wideband rf amplifier esebenza phakathi kwe-500 MHz kunye ne-2700 MHz, inamandla okufumana i-43dB kunye namandla okukhupha angama-20 watts, kwaye isebenza kakuhle kwi-UHF band.
Izihlanganisi zomdibaniso wokufaka kunye nokukhupha zale amplifier ye-wideband rf zizihlanganisi zabasetyhini ze-SMA, ezifanelekileyo kuluhlu lweefrikhwensi ukuya kuthi ga kwi-26.5 GHz, zibonelela ngeenzuzo ze-bandwidth ebanzi, ukusebenza okugqwesileyo, ukuthembeka okuphezulu kunye nobomi obude.
Ubushushu bokusebenza be-wideband rf amplifier bunokuqala kwi -40 degrees Celsius ukuya kwi 60 degrees Celsius. Ubushushu bokugcina bungafikelela kwi minus 45 degrees Celsius kwaye imozulu eshushu ifikelele kwi 85 degrees Celsius. Ubushushu obuhambelanayo buyahambelana neendawo ezininzi zengingqi, kwaye bungasetyenziswa kwi 95% okanye ngaphantsi.
I-amplifier ye-rf ye-wideband ye-Mars RF ingasetyenziswa kwi-RF jamming, i-gallium nitride radar, unxibelelwano, uvavanyo kunye nokulinganisa (njenge-EMI EMC, njl.njl.), kunye neminye imimandla yorhwebo kunye neyemizi-mveliso. Ii-amplifier ze-rf ze-wideband ze-RF ze-Mars' zinokuguquguquka okuphezulu kunye nokukwazi ukuzenza ngokwezifiso, ezinokuhlangabezana neemfuno zamashishini ahlukeneyo kunye nezicelo, kwaye zibonelele ngezisombululo zemveliso ye-RF ezinokuthenjwa.
Sibonelela abathengi ngee-heat sinks ezikhethwayo. Ii-heat sinks ezikumgangatho ophezulu zeMars RF zivumela i-wideband rf amplifier ukuba igcine ukusebenza okuphezulu phantsi kweemeko ezahlukeneyo, iphucule ukusebenza kakuhle, kwaye inciphise ukuphindaphindeka kunye neendleko zokugcinwa kwenkqubo.

Ezona mpawu

√ Uyilo oluthe tyaba lweClass AB oluqinileyo
√ I-broadband ekhawulezayo ekhawulezayo
√ Incinci kwaye ilula
√ Ifanelekile kwi-CW, AM, kunye ne-FM, njl.
√ Ukuthembeka okuphezulu kunye nokuqina

FAQ

Ingakanani amandla emveliso eMars RF?
I-Mars RF inezixhobo zokuvelisa eziphambili kunye neqela leenjineli ezinamava. Ifektri yethu ye-SSPA inemigca yemveliso eli-10, emibini yayo yimigca yegumbi elicocekileyo. Le migca yemveliso esemgangathweni ayiqinisekisi nje kuphela ukusebenza kakuhle kwemveliso yethu kunye nokuhanjiswa ngokukhawuleza, kodwa kunye nemigca yemveliso yegumbi elicocekileyo inokuhlangabezana neemfuno zokuhanjiswa ezisemgangathweni ophezulu zabathengi bethu.
Zithini iingenelo zezihlanganisi ze-SMA plug ezisetyenziswa kwi-wideband rf amplifiers?
Imisebenzi eqhelekileyo kunye neendima zezihlanganisi ze-SMA ziquka.
1. Ukuphazamiseka okuphantsi, okunokubonelela ngonxibelelwano oluthembekileyo loomatshini.
2. I-broadband ekhawulezayo
3.Impedance ephezulu ene-50 ohm impedance ukuze ihambelane nezixhobo ezininzi zeRF ezisetyenziswa rhoqo.
4. Uyilo oluncinci, olufanelekileyo kwiisekethe zeRF ezincinci ezidityanisiweyo kakhulu kunye nezixhobo.
5. Ngokumelana nobushushu obuphezulu.
Ngamafutshane, isixhumi se-SMA sisixhumi esibalulekileyo se-RF, umsebenzi kunye nendima yaso inokunceda ekufezekiseni ukuhanjiswa kwesignali ye-RF kunye nonxibelelwano lwedatha olusebenzayo.

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