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  • Ibhendi eBanzi yeNgxolo ePhantsi Ubushushu boNgeniso oluPhantsi lwe-VSWR iSatcom iAmplifaya yeNgxolo ePhantsi
  • Ibhendi eBanzi yeNgxolo ePhantsi Ubushushu boNgeniso oluPhantsi lwe-VSWR iSatcom iAmplifaya yeNgxolo ePhantsi
  • Ibhendi eBanzi yeNgxolo ePhantsi Ubushushu boNgeniso oluPhantsi lwe-VSWR iSatcom iAmplifaya yeNgxolo ePhantsi

    Iimbonakalo:

    • Broadband
    • Ubushushu obuphantsi bengxolo
    • Igalelo eliphantsi VSWR

    Usetyenziso:

    • Isitishi esisisigxina
    • Isitishi esiphathwayo
    • Uvavanyo lweLebhu

    I-Satcom Low Noise Amplifiers zizinto eziphambili kwiinkqubo zonxibelelwano ngesathelayithi. Umsebenzi wabo ophambili kukukhulisa imiqondiso ebuthathaka efunyenwe kwiisathelayithi ngelixa unciphisa ukuqaliswa kwengxolo.

    Injongo:

    1. Ukwandiswa koMqondiso: Umsebenzi ophambili we-Satcom Low Noise Amplifiers kukukhulisa imiqondiso ebuthathaka efunyenwe kwiisathelayithi ukuze kufumaneke amandla okwaneleyo okusetyenzwa komqondiso olandelayo kunye nokuhanjiswa.
    2. Ukunciphisa Ingxolo: Injongo ephambili ekuyilweni kwe-Satcom Low Noise Amplifiers kukunciphisa ingxolo eyaziswa ngexesha lenkqubo yokukhulisa, ngaloo ndlela iphucula i-signal-to-noise ratio (SNR) yomqondiso. Oku kubaluleke ngakumbi ekufumaneni imiqondiso yesathelayithi ebuthathaka.
    3. Ukulungelelaniswa kweRange Range: I-Satcom Low Noise Amplifiers idla ngokuyilwa kwiintlobo ezithile zefrikhwensi, ezifana ne-C-band, i-Ku-band, okanye i-Ka-band, ukuqinisekisa ukusebenza kakuhle kunye nokuhambelana.

    Isicelo:

    1. Umabonakude wesathelayithi: Kwiinkqubo zesathelayithi zokwamkela umabonakude, iSatcom Low Noise Amplifiers isetyenziselwa ukukhulisa isignali yeTV efunyenwe kwisathelayithi. Zihlala zidityaniswe kwii-low-noise downconverters (LNBs), ezinceda ukuphucula umgangatho wesignali kunye nokwenza ukuba abamkeli bahlule kwaye babonise umxholo wethelevishini.
    2. I-Intanethi yeSathelayithi: Kwiinkqubo ze-Intanethi zesathelayithi, iSatcom Low Noise Amplifiers isetyenziselwa ukukhulisa imiqondiso yedatha efunyenwe kwiisathelayithi. Ukwandiswa komgangatho ophezulu wesignali kunceda ukwandisa amazinga okudlulisa idatha kunye nokuzinza koqhagamshelwano.
    3. UNxibelelwano ngeSathelayithi: I-Satcom Low Noise Amplifiers isetyenziswa kakhulu kwiinkqubo ezahlukeneyo zonxibelelwano ngesathelayithi, kubandakanywa neefowuni zesathelayithi, ukuhanjiswa kwedatha, kunye neenkomfa ngevidiyo. Banceda ukukhulisa iimpawu zonxibelelwano ezifunyenweyo, ukuphucula ukuthembeka kunye nomgangatho wonxibelelwano lonxibelelwano.
    4. Ukujongwa koMhlaba kunye nokuVavanya okuLawulwa kude: Kuphononongo loMhlaba kunye nezicelo zokuvalelwa kude, iSatcom Low Noise Amplifiers isetyenziselwa ukukhulisa idatha yeremote sensing efunyenwe kwiisathelayithi. Ezi nkcukacha zingasetyenziswa kwiindawo ezifana nokubeka iliso kwimozulu, ukubeka iliso kokusingqongileyo kunye nesilumkiso sentlekele.
    5. Izicelo zoShishino kunye nezoRhwebo: Imibutho emininzi yamashishini kunye nezorhwebo isebenzisa unxibelelwano lwesathelayithi ukujonga kude, ukuhanjiswa kwedatha, kunye nezinye izicelo.

    I-Satcom Low Noise Amplifiers inceda ukuphucula umgangatho wesignali kunye nokuthembeka kwezi nkqubo.

    Qualwaveinikeza iintlobo ezahlukeneyo ze-Satcom Low Noise Amplifiers kwi-Ka, Ku, L, P, S, C-Band, kunye nobushushu bengxolo ye-40 ~ 170K. Ukupheliswa kunye neentlobo ezahlukeneyo ukuhlangabezana neemfuno zabathengi.

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    I-Satcom Low Noise Amplifiers
    Inombolo yendawo Ibhendi Ukuphindaphinda (GHz) NT(K) P1dB (dBm, Min.) Inzuzo (dB) Ukufumana ukuFileka (±dB, max.) Isidibanisi Umbane (DC) I-VSWR (Ubukhulu.) Ixesha lokukhokela (iiveki)
    QSLA-200-400-30-45 P 0.2~0.4 45 10 30 0.5 N, SMA 15 1.5/1.5 2~8
    QSLA-200-400-50-45 P 0.2~0.4 45 10 50 0.5 N, SMA 15 1.5/1.5 2~8
    QSLA-950-2150-30-50 L 0.95~2.15 50 10 30 0.8 N, SMA 15 1.5/1.5 2~8
    QSLA-950-2150-50-50 L 0.95~2.15 50 10 50 0.8 N, SMA 15 1.5/1.5 2~8
    QSLA-2200-2700-30-50 S 2.2~2.7 50 10 30 0.75 N, SMA 15 2.0/1.5 2~8
    QSLA-2200-2700-50-50 S 2.2~2.7 50 10 50 0.75 N, SMA 15 2.0/1.5 2~8
    QSLA-3400-4200-60-40 C 3.4~4.2 40 10 60 0.75 I-WR-229(BJ40), N, SMA 15 1.35/1.5 2~8
    QSLA-7250-7750-60-70 X 7.25~7.75 70 10 60 0.75 I-WR-112(BJ84), N, SMA 15 1.35/1.5 2~8
    QSLA-8000-8500-60-80 X 8~8.5 80 10 60 0.75 I-WR-112(BJ84), N, SMA 15 2.0/1.5 2~8
    QSLA-10700-12750-55-80 Ku 10.7~12.75 80 10 55 1.0 I-WR-75(BJ120), N, SMA 15 2.5/1.5 2~8
    QSLA-11400-12750-55-60 Ku 11.4~12.75 60 10 55 0.75 I-WR-75(BJ120), N, SMA 15 2.5/1.5 2~8
    QSLA-17300-22300-55-170 Ka 17.3~22.3 170 10 55 2.5 I-WR-42(BJ220), 2.92mm, SSMA 15 2.5/2.0 2~8
    QSLA-17700-21200-55-150 Ka 17.7~21.2 150 10 55 2.0 I-WR-42(BJ220), 2.92mm, SSMA 15 2.5/2.0 2~8
    QSLA-19200-21200-55-130 Ka 19.2~21.2 130 10 55 1.5 I-WR-42(BJ220), 2.92mm, SSMA 15 2.5/2.0 2~8
    Anti 5G Interference LNAs
    Inombolo yendawo Ibhendi Ukuphindaphinda (GHz) NT(K) P1dB (dBm, Min.) Inzuzo (dB) Ukufumana ukuFileka (±dB, max.) Isidibanisi Umbane (DC) I-VSWR (Ubukhulu.) Ixesha lokukhokela (iiveki)
    QSLA-3625-4200-60-50 C 3.625~4.2 50 10 60 2.0 I-WR-229 (BJ40), N, SMA 15 2.5/2.0 2~8
    QSLA-3700-4200-60-50 C 3.7~4.2 50 10 60 2.0 I-WR-229 (BJ40), N, SMA 15 2.5/2.0 2~8

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