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Aanpasbare Multi IR Breëbandfilter van China Verskaffers en Fabriek - Hoë Werkverrigting vir Optiese Toepassings
| Produknaam | 50% SNY LINKS | 50% SNY AAN REGS | HPB(nm) | Hoë-deursigtigheidsarea | Tmin | Tavg | Grootte (mm) | Submateriaal | Blokkering | Tmaks | Tavg | Spektrogram |
| WBP850~2650 | 1000~2500 | / | ≥90 | Φ0.1~300 | Saffier |
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| WBP970~2470 | 900 | 2400 | / | 1100~2300 | / | ≥85 | Φ0.1~300 | D263T | 200~3500 |
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| WBP1000~3000 | 970 | 2470 | / | 1100~2300 | / | ≥90 | Φ0.1~300 | Glaskeramiek | 200~3560 |
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| WBP1520~1850 | 1520 | 1850 | / | 1600~1750 | / | ≥80 | Φ0.1~300 | En | 400~3300 |
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| WBP1550~1750 | 1550 | 1750 | / | 1600~1700 | / | ≥80 | Φ0.1~300 | En | 1500~2800 |
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| WBP1550~5050 | 1550 | 5050 | / | 1600~5000 | / | ≥80 | Φ0.1~300 | En | 1500~5580 |
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| WBP1615~2735 | 1650~2700 | / | ≥85 | Φ0.1~300 | JGS3 | 400~1550 |
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| WBP1650~2350 | 1650 | 2350 | / | 1700~2250 | / | ≥80 | Φ0.1~300 | En | 400~4000 |
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| WBP1900~2250 | 1900 | 2250 | / | 2000~2150 | / | ≥80 | Φ0.1~300 | En | 1500~5000 |
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| WBP2000~2400 | 2000 | 2400 | / | 2080~2330 | / | ≥75 | Φ0.1~300 | Wit Glas | 400~6500 |
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| WBP2050~2350 | 2050 | 2350 | / | 2150~2250 | / | ≥80 | Φ0.1~300 | En | 1500~2800 |
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| WBP2050~2500 | 2050 | 2500 | / | 2150~2450 | / | ≥80 | Φ0.1~300 | En | 1500~5000 |
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| WBP2080~2350 | 2080 | 2350 | / | 2135~2330 | / | ≥80 | Φ0.1~300 | En | 1500~2800 |
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| WBP2080~2430 | 2080 | 2430 | / | 2180~2330 | / | ≥80 | Φ0.1~300 | En | 1500~2800 |
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| WBP2170~3670 | 2170 | 3670 | / | 2300~3600 | / | ≥85 | Φ0.1~300 | En | 1500~5000 |
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| WBP2250~3810 | 2250 | 3810 | / | 2340~3670 | / | ≥80 | Φ0.1~300 | En | 1500~5000 |
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| WBP2300~3600 | 2200 | 3750 | / | 2300~3600 | / | ≥85 | Φ0.1~300 | En | 1500~5000 |
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| WBP2300~3700 | 2250 | 3770 | / | 2300~3700 | / | ≥90 | Φ0.1~300 | En | 1500~5000 |
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| WBP2350~2750 | 2400~2700 | / | ≥80 | Φ0.1~300 | En | 400~6000 |
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| WBP2400~3150 | 2400 | 3150 | 2500~3000 | / | ≥90 | Φ0.1~300 | Saffier | 400~10500 |
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| WBP2430~5150 | 2500~4800 | / | ≥90 | Φ0.1~300 | Saffier | 5250~7000 |
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| WBP2450~4600 | 2450 | 4600 | / | 2550~4500 | / | ≥90 | Φ0.1~300 | Ge | 400~7000 |
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| WBP2450~3200 | 2450 | 3200 | / | 2500~3140 | / | ≥90 | Φ0.1~300 | Ge | 1500~7000 |
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| WBP2450~5150 | 2450 | 5150 | / | 2640~5040 | / | ≥90 | Φ0.1~300 | En | 400~7040 |
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| WBP2490~5240 | 2490 | 5240 | / | 2640~5040 | / | ≥90 | Φ0.1~300 | En | 400~7040 |
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| WBP2500~5000 | 2500 | 5000 | 2700~4900 | / | ≥90 | Φ0.1~300 | Ge | 200~10000 |
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| WBP2500~5100 | 2500 | 5100 | 2650~4950 | / | ≥90 | Φ0.1~300 | Ge | 1500~10500 |
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| WBP2500~5400 | 2500 | 5400 | 2600~5250 | / | ≥85 | Φ0.1~300 | Saffier | 400~14000 |
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| WBP2550~3100 | 2550 | 3100 | / | 2650~3000 | / | ≥90 | Φ0.1~300 | En | 1500~5000 | 1.5 |
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| WBP2550~3150 | 2550 | 3150 | / | 2700~3100 | / | ≥85 | Φ0.1~300 | En | 1500~5000 | 1.5 |
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| WBP2550~3250 | 2550 | 3250 | / | 2700~3100 | / | ≥90 | Φ0.1~300 | En | 430~10030 |
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| WBP2550~3300 | 2550 | 3300 | / | 2800~3000 | / | ≥90 | Φ0.1~300 | Saffier | 400~20000 |
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| WBP2600~3200 | 2600 | 3200 | / | 2700~3100 | / | ≥85 | Φ0.1~300 | Ge | 1500~5000 |
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| WBP2600~3250 | 2600 | 3250 | / | 2700~3200 | / | ≥90 | Φ0.1~300 | Ge | 1500~5000 | 8 |
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| WBP2600~3300 | 2600 | 3300 | / | 2850~3000 | / | ≥85 | Φ0.1~300 | Ge | 400~10000 |
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| WBP2600~5000 | 2490 | 5240 | 2640~5040 | / | ≥90 | Φ0.1~300 | Ge | 400~7040 |
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| WBP2650~3000 | 2650 | 3000 | 2700~2950 | / | ≥85 | Φ0.1~300 | Ge | 1000~6000 |
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| WBP2650~5050 | 2600 | 5050 | 2750~4950 | / | ≥90 | Φ0.1~300 | En | 1500~8000 |
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| WBP2700~3150 | 2700 | 3150 | / | 2800~3050 | / | ≥80 | Φ0.1~300 | Ge | 1500~5000 |
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| WBP2700~2950 | 2700 | 2950 | / | 2750~2900 | / | ≥85 | Φ0.1~300 | En | 1500~6500 |
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| WBP2700-3550 | 2700 | 3550 | / | 2800~3450 | / | ≥90 | Φ0.1~300 | Saffier | 300~20000 |
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| WBP2700-3600 | 2700 | 3600 | / | 2800~3500 | / | ≥90 | Φ0.1~300 | Saffier | 300~20000 |
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| WBP2720~2980 | 2720 | 2980 | / | 2780~2920 | / | ≥80 | Φ0.1~300 | Ge | 1500~5000 |
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| WBP2730~3010 | 2730 | 3010 | / | 2800~2900 | / | ≥85 | Φ0.1~300 | Ge | 1500~5000 |
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| WBP2750~4850 | 2750 | 4850 | 3000~4600 | / | ≥85 | Φ0.1~300 | Ge | 1000~5100 |
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| WBP2750~2950 | 2750 | 2950 | / | 2800~2900 | / | ≥85 | Φ0.1~300 | En | 1500~6500 |
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| WBP2750~5100 | 2750 | 5100 | 2900~5000 | / | ≥90 | Φ0.1~300 | Ge | 1500~10500 |
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| WBP2790~3070 | 2790 | 3070 | / | 2900~3000 | / | ≥80 | Φ0.1~300 | Ge | 1500~5000 |
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| WBP2800~3050 | 2800 | 3050 | / | 2900~3000 | / | ≥90 | Φ0.1~300 | En | 1500~6500 |
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| WBP2800~5150 | 2800 | 5150 | / | 2950~5000 | / | ≥90 | Φ0.1~300 | Ge | 1500~10500 |
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| WBP2800~5200 | 2800 | 5200 | / | 2950~5050 | / | ≥90 | Φ0.1~300 | Ge | 1500~10500 |
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| WBP 2800~5200 eenhede | 2800 | 5200 | 2900~5100 | ≥55 | Φ0.1~300 | En | 2580~8000 |
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| WBP2800~5250 | 2800 | 5250 | 2950~5100 | / | ≥90 | Φ0.1~300 | Ge | 1500~10500 |
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| WBP2850~4150 | 3000~4000 | / | ≥90 | Φ0.1~300 | Saffier | 400~11000 |
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| WBP2850~5150 | 2850 | 5150 | / | 3000~5000 | / | ≥85 | Φ0.1~300 | Ge | 1500~10500 |
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| WBP2900~4140 | 2900 | 4140 | / | 3100~4040 | / | ≥90 | Φ0.1~300 | Ge | 700~8040 |
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| WBP2900~4450 | 2900 | 4450 | 3050~4350 | / | ≥85 | Φ0.1~300 | Ge | 1500~10000 |
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| WBP2900~4550 | 2900 | 4550 | 3050~4450 | / | ≥85 | Φ0.1~300 | Ge | 1500~10000 |
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| WBP2900~4850 | 2900 | 4850 | 3050~4750 | / | ≥90 | Φ0.1~300 | En | 400~11000 |
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| WBP2900~4900 | 2800 | 3750 | 2900~3500 | / | ≥90 | Φ0.1~300 | Saffier | 190~5500 |
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| WBP2900~5100 | 2900 | 5100 | / | 3000~5000 | / | ≥90 | Φ0.1~300 | Ge | 1000~10500 |
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| WBP2950~3600 | 2950 | 3600 | / | 3150~3400 | / | ≥85 | Φ0.1~300 | Ge | 1000~10500 |
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| WBP2950~3650 | 2950 | 3650 | / | 3150~3450 | / | ≥85 | Φ0.1~300 | Ge | 1000~10500 |
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| WBP2950~3250 | 2950 | 3250 | / | 3000~3200 | / | ≥85 | Φ0.1~300 | Saffier | 200~20000 |
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| WBP2950~4950 | 2950 | 4950 | 3100~4800 | / | ≥90 | Φ0.1~300 | En | 400~11000 |
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| WBP2950~5250 | 3000 | 5400 | / | 3100~5300 | / | ≥85 | Φ0.1~300 | Ge | 1500~7000 |
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| WBP3000~3300 | 3000 | 3300 | / | 3050~3250 | / | ≥85 | Φ0.1~300 | Saffier | 200~20000 |
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| WBP3000~3500 | / | / | 480 | 3050~3400 | / | ≥80 | Φ0.1~300 | Kwarts | 300~6500 |
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| WBP3000~3700 | 3000 | 3700 | 3100~3600 | / | ≥90 | Φ0.1~300 | Ge | 200~10000 |
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| WBP3000~3800 | 3000 | 3800 | / | 3100~3700 | / | ≥80 | Φ0.1~300 | Saffier | 400~14000 |
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| WBP3000~3875 | 3000 | 3875 | / | 3250~3650 | / | ≥80 | Φ0.1~300 | Saffier | 500~5500 |
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| WBP3000~4260 | 3000 | 4260 | 3250~3900 | / | ≥80 | Φ0.1~300 | En | 400~11000 |
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| WBP3000~4300 | 3000 | 4300 | 3250~3900 | / | ≥80 | Φ0.1~300 | En | 400~11000 |
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| WBP3000~5000 | 3000 | 5000 | / | 3100~4900 | / | ≥85 | Φ0.1~300 | En | 1500~11000 |
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| WBP3000~5300 | 3000 | 5300 | / | 3150~5150 | / | ≥85 | Φ0.1~300 | Saffier | 1500~15500 |
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| WBP3000~5400 | 3000 | 5400 | 3100~5300 | / | ≥90 | Φ0.1~300 | Ge | 1500~2800 |
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| WBP3020~3320 | 3020 | 3320 | 3050~3250 | / | ≥85 | Φ0.1~300 | Saffier | 200~20000 |
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| WBP3040~4320 | 3040 | 4320 | 3250~4050 | / | ≥85 | Φ0.1~300 | En | 400~11000 |
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| WBP3050~4200 | 3050 | 4200 | 3250~3900 | / | ≥85 | Φ0.1~300 | En | 400~11000 |
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| WBP3050~5450 | 3050 | 5450 | / | 3200~5300 | / | ≥85 | Φ0.1~300 | Saffier | 1500~15500 |
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| WBP3050~5000 | 3050 | 5000 | / | 3200~4850 | / | ≥85 | Φ0.1~300 | En | 1500~10000 |
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| WBP3100~3700 | 3100 | 3700 | 3200~3600 | / | ≥90 | Φ0.1~300 | Saffier | 400~20000 |
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| WBP3100~4100 | 3100 | 4100 | 3300~3900 | / | ≥90 | Φ0.1~300 | Ge | 900~8000 |
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Die bogenoemde lys toon ons huidige voorraaditems.
Indien u nie sien waarna u soek nie, asseblief kontak ons.
Gereelde vrae (FAQ)
V1: Waarvoor word wye banddeurlaatfilters (WBP-filters) gebruik?
Breëbanddeurlaatfilters is ontwerp om 'n breë spektrum lig deur te dra terwyl ongewenste golflengtes buite die deurlaatband hoogs geblokkeer word. Hulle word algemeen gebruik in infrarooibeelding, gasanalise, spektroskopie en omgewingsmoniteringstoepassings.
V2: Watter substraatmateriale is beskikbaar vir hierdie optiese filters?
Afhangende van jou teikengolflengtebereik, bied ons filters vervaardig op saffier, silikon (Si), germanium (Ge), sinkselenied (ZnSe), kwarts en glaskeramiek om optimale transmissie en duursaamheid te verseker.
V3: Kan ek 'n persoonlike grootte of vorm vir my filter aanvra?
Ja, ons standaard vervaardigingsgrootte-vermoëns wissel van Φ0.1 mm tot 300 mm. Ons kan afmetings, vorms en randprofiele (insluitend wigvormige substrate) aanpas om by u spesifieke instrumentkonfigurasies te pas.
V4: Wat is die tipiese transmissietempo (Tavg) en blokkeringsprestasie?
Die meeste van ons standaardfilters beskik oor gemiddelde transmissievlakke (Tavg) van ≥80% of ≥90% in die hoë-deursigtigheidsarea, met diep blokkeringsprestasie wat buite-band-transmissie tot minder as 1% (
V5: Hoe kies ek tussen Silikon (Si) en Germanium (Ge) substrate?
Silikon word tipies verkies vir die 1.5 µm tot 6 µm naby-tot-middel infrarooi reeks as gevolg van sy ligter gewig en laer koste. Germanium is ideaal vir langer infrarooi toepassings (tot 12 µm en verder) en omgewings wat 'n hoë brekingsindeks vereis.
V6: Wat moet ek doen as 'n spesifieke spesifikasie nie in u voorraad gelys word nie?
Indien u persoonlike optiese spesifikasies benodig, klik asseblief op die "kontak ons"-skakel om met ons ingenieurspan in verbinding te tree. Ons bied persoonlike dunfilmbedekkingsontwerpe en substraatvervaardiging om aan u unieke projekvereistes te voldoen.







