MW princeps | Introductio ad cohortem subsisto filter |
Cohors subsisto Filtra, etiam notum ut cohortem subsisto Filtra, sunt amet instrumenta in electronics et telecommunications. Et facultatem ad supprimere unwanted frequentiis in certa range facit eam magni momenti pars applications ut audio processui, radio frequency intercessiones mitigandis, et biomedical signo analysis.
Nostrum Bandstop Filtra providere uniceed accurate et perficientur, ensuring quod solum frequency components of interest sunt suppressae dum maintaining altiore signi integritas. Hoc gradu accuratissime est critica in condicionibus, ubi praesentia de quadam frequenciis degrades signum qualis vel intermingat cum desideravit output.
Unum de principalis commoda nostrae cohortis subsisto Filtra est eorum versatility. Potest esse in unamquam integrated in varietate systems et cogitationes, inter audio apparatu, communicationis retiacula, et medicinae instrumenta. Utrum vos es opus in audio productio, wireless communications vel physiologica magna, nostri cohortis subsisto Filtra providere certa solutio ad administrandi invitis frequency components.
Praeterea, nostri Bandstop Filtra sunt machinatum providere consistent et reliable perficientur, cursus diu terminus stabilitatem et diuturnitatem. Et robust consilio et altus-qualitas components faciunt idoneam ad postulantes industriae applications tum R & D projects.
In summary, nostrum Bandstop Filtra Repraesentare a breakthrough in signum processus technology, providente precise et effective attenuatione specifica frequency components. Et eius versatility et reliability, idealis est ad professionales et investigatores quaerens summus perficientur solutions ad administrandi frequency intercessiones. Usus difference nostri Bandstop Filtra et recludam plenus potential tua signo dispensando applications.
MW princeps | Specificatio |
Pars numerus | Subsisto cohortem (MHZ) | Pass Band | Insertionem damnum (DB) | Band Transite VSWR | Type COPULATOR | Subsisto cohortem rejectionem | Dimensiones (mm) |
LBT-DCCCLXXX / CMLX Q9s | 880-960 | 10MHz-700MHz & 1200-2100MHz | ≤3.0db | ≤1.6 | SMA-F | ≥30db @ 880-960mhz | CCCX * LXV * XXX |
LBT, MCDXXXVII / 1467-2s | 1437-1467 | DC, 1347MHz & 1550-2400MHz | ≤3.0db | ≤1.6 | SMA-F | ≥50db @ 1437-1467MHz | CCLII * LXIII * XXVI |
LBT-MDCCLXXXV / 1805-2s | 1785-1805 | DC-1700MHz & 1885-2600MHz | ≤3.0db | ≤1.6 | SMA-F | ≥50db @ 1785-1805MHz | CCLII * LXI * XXVI |
LBT, 1842,5 / 75-2s | MDCCCV ~ MDCCCLXXX | DC ~ 1795MHz & 1890-3600MHz | ≤2.0db | ≤1.8 | SMA-F | ≥40db @ MDCCCV ~ 1880mhz | CDLXIV * LXI * XXVI |
LBT, MDCCCLXXX / 1920-2s | 1880-1920 | DC, 1800MHz & 2000-3000MHz | ≤3.0db | ≤1.6 | SMA-F | ≥50db @ 1880-1920MHz | CCLII * LXI * XXVI |
LTF-MMCDXX / 2470-2s | 2420-2470 | DC, 2400MHz & 2490-4000MHz | ≤4.5db | ≤1.8 | SMA-F | ≥50db @ 2420-2470MHz | CLXXXII * L * XXXI |
LTF-MMDLXXV / 2595-1 | 2575-2595 | 800-2400MHz 2605-3000MHz | ≤3db | ≤1.68 | SMA-F | ≥20db @ 2575-2595MHz | CCXCVI * LXXIV * LVIII |
LTF-(V) CL / 5925-2s | 5150-5925 | DC-5000MHz & 6105-8000MHz | ≤4.5db | ≤1.8 | SMA-F | ≥40DB @ 5150-5925MHz | 79.3 * 25.2 * XIII |
LTF-(V) CL / (V) CCL, Q7 | 5150-5250 | DC-5120MHz & 5280-8000MHz | ≤3.5db | ≤2.0 | NY | ≥40DB @ 5150-5250MHz | CXVI * 28.4 * XX |
LTF-(V) CCL / (V) CCCL Q7 | 5250-5350 | DC-5220MHz & 5380-8000MHz | ≤3.5db | ≤2.0 | NY | ≥40DB @ 5250-5350MHz | CXVI * 28.4 * XX |
LTF-(V) DCCXXV / (V) DCCCXXV-Q7 | 5725-5825 | DC-5695MHz & 5855-8000MHz | ≤3.5db | ≤2.0 | NY | ≥40DB @ 5725-5825MHz | CXVI * 28.4 * XX |
LTF-(V) CDLXX / (V) DCCXXV, Q7 | 5470-5725 | DC-5430MHz & 5765-8000MHz | ≤3.5db | ≤2.0 | NY | ≥40DB @ 5470-5725MHz | CXVI * 28.4 * XX |