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Matatar Watsa Labarai ta IR Mai Yawa da Za a Iya Keɓancewa Daga Masu Kaya & Masana'antu na China - Babban Aiki Don Aikace-aikacen gani
Kayayyakin Zafi
Nau'o'in Kayayyaki
Kayayyakin da aka Fito
Matatar Tsawon IR (LP)

Matatar Tsawon IR (LP)
Matatar Wayar Hannu ta IR (WBP)

Matatar Wayar Hannu ta IR (WBP)
Matatar Narrowband ta Infrared (BP)

Matatar Narrowband ta Infrared (BP)
Rufin Matatar Hana Nuna Hasken Infrared (AR)

Rufin Matatar Hana Nuna Hasken Infrared (AR)
Rufin Matatar Carbon Mai Kama da Lu'u-lu'u (DLC)

Rufin Matatar Carbon Mai Kama da Lu'u-lu'u (DLC)
Matatar Rarraba Hasken Infrared (BS)

Matatar Rarraba Hasken Infrared (BS)
Matatar Tashar Infrared Biyu (BP+BP)

Matatar Tashar Infrared Biyu (BP+BP)
Matatar Tashar Infrared Biyu (WBP+LP)

Matatar Tashar Infrared Biyu (WBP+LP)
Matatar Tashar Infrared Biyu (WBP+WBP)

Matatar Tashar Infrared Biyu (WBP+WBP)
Rufin AR

Rufin AR
0102030405
Tace Mai Rufe IR WBP (1).jpg
Tace Mai Rufe IR WBP (2).jpg
Tace Mai Rufe IR WBP (3).jpg

Matatar Watsa Labarai ta IR Mai Yawa da Za a Iya Keɓancewa Daga Masu Kaya & Masana'antu na China - Babban Aiki Don Aikace-aikacen gani

Gabatar da Matatar Broadband ta MULTI IR, wani babban samfuri daga shahararrun masu samar da kayayyaki da masana'antun China. An tsara wannan matatar mai ci gaba da fa'idodi masu yawa kamar fa'idodi masu yawa, watsawa mai faɗi a cikin madaurin wucewa, zurfin yankewa mai zurfi, da kuma tsayin gefen gaba. Ana amfani da shi sosai a aikace-aikacen gani daban-daban, gami da nazarin iskar gas, auna zafin jiki na infrared, gwajin likita, da tsarin tsaro. Masana'antarmu tana ba da zaɓuɓɓukan keɓancewa don kewayon madaurin wucewa, tsawon yankewa, girma, da sigogin kallo, tabbatar da cewa za ku iya daidaita matatar don biyan buƙatun ƙira na musamman na tsarin gani. Gano inganci da amincin Matatar Broadband ta MULTI IR, wacce aka ƙera don haɓaka ayyukanku.
    Tuntube mu

    Sunan Samfuri A YANKE 50% A HAGU 50% A RAGE A DAMA HPB(nm) Yankin bayyanannen abu Tmin Tavg Girman (mm) Ƙananan kayan aiki Toshewa Tmax Tavg Spectrogram
    WBP850~2650 1000~2500 / ≥90 Φ0.1~300 Saffir
    Spectrogram
    WBP970~2470 900 2400 ／ 1100~2300 / ≥85 Φ0.1~300 D263T 200~3500
    Spectrogram
    WBP1000~3000 970 2470 ／ 1100~2300 / ≥90 Φ0.1~300 Gilashin Yumbu 200~3560
    Spectrogram
    WBP1520~1850 1520 1850 ／ 1600~1750 / ≥80 Φ0.1~300 Kuma 400~3300
    Spectrogram
    WBP1550~1750 1550 1750 ／ 1600~1700 / ≥80 Φ0.1~300 Kuma 1500~2800
    Spectrogram
    WBP1550~5050 1550 5050 ／ 1600~5000 / ≥80 Φ0.1~300 Kuma 1500~5580
    Spectrogram
    WBP1615~2735 1650~2700 / ≥85 Φ0.1~300 JGS3 400~1550
    Spectrogram
    WBP1650~2350 1650 2350 ／ 1700~2250 / ≥80 Φ0.1~300 Kuma 400~4000
    Spectrogram
    WBP1900~2250 1900 2250 ／ 2000-2150 / ≥80 Φ0.1~300 Kuma 1500~5000
    Spectrogram
    WBP2000~2400 2000 2400 ／ 2080-2330 / ≥75 Φ0.1~300 Gilashin Fari 400~6500
    Spectrogram
    WBP2050~2350 2050 2350 ／ 2150~2250 / ≥80 Φ0.1~300 Kuma 1500~2800
    Spectrogram
    WBP2050~2500 2050 2500 ／ 2150~2450 / ≥80 Φ0.1~300 Kuma 1500~5000
    Spectrogram
    WBP2080~2350 2080 2350 ／ 2135~2330 / ≥80 Φ0.1~300 Kuma 1500~2800
    Spectrogram
    WBP2080~2430 2080 2430 ／ 2180~2330 / ≥80 Φ0.1~300 Kuma 1500~2800
    Spectrogram
    WBP2170~3670 2170 3670 ／ 2300~3600 / ≥85 Φ0.1~300 Kuma 1500~5000
    Spectrogram
    WBP2250~3810 2250 3810 ／ 2340~3670 / ≥80 Φ0.1~300 Kuma 1500~5000
    Spectrogram
    WBP2300~3600 2200 3750 ／ 2300~3600 / ≥85 Φ0.1~300 Kuma 1500~5000
    Spectrogram
    WBP2300~3700 2250 3770 ／ 2300~3700 / ≥90 Φ0.1~300 Kuma 1500~5000
    Spectrogram
    WBP2350~2750 2400~2700 / ≥80 Φ0.1~300 Kuma 400~6000
    Spectrogram
    WBP2400~3150 2400 3150 2500~3000 / ≥90 Φ0.1~300 Saffir 400~10500
    Spectrogram
    WBP2430~5150 2500~4800 / ≥90 Φ0.1~300 Saffir 5250~7000
    Spectrogram
    WBP2450~4600 2450 4600 / 2550~4500 / ≥90 Φ0.1~300 Ge 400~7000
    Spectrogram
    WBP2450~3200 2450 3200 ／ 2500~3140 / ≥90 Φ0.1~300 Ge 1500~7000
    Spectrogram
    WBP2450~5150 2450 5150 ／ 2640~5040 / ≥90 Φ0.1~300 Kuma 400~7040
    Spectrogram
    WBP2490~5240 2490 5240 ／ 2640~5040 / ≥90 Φ0.1~300 Kuma 400~7040
    Spectrogram
    WBP2500~5000 2500 5000 2700~4900 / ≥90 Φ0.1~300 Ge 200~10000
    Spectrogram
    WBP2500~5100 2500 5100 2650~4950 / ≥90 Φ0.1~300 Ge 1500~10500
    Spectrogram
    WBP2500~5400 2500 5400 2600~5250 / ≥85 Φ0.1~300 Saffir 400~14000
    Spectrogram
    WBP2550~3100 2550 3100 ／ 2650~3000 / ≥90 Φ0.1~300 Kuma 1500~5000 1.5
    Spectrogram
    WBP2550~3150 2550 3150 ／ 2700~3100 / ≥85 Φ0.1~300 Kuma 1500~5000 1.5
    Spectrogram
    WBP2550~3250 2550 3250 ／ 2700~3100 / ≥90 Φ0.1~300 Kuma 430~10030
    Spectrogram
    WBP2550~3300 2550 3300 ／ 2800~3000 / ≥90 Φ0.1~300 Saffir 400~20000
    Spectrogram
    WBP2600~3200 2600 3200 ／ 2700~3100 / ≥85 Φ0.1~300 Ge 1500~5000
    Spectrogram
    WBP2600~3250 2600 3250 ／ 2700~3200 / ≥90 Φ0.1~300 Ge 1500~5000 8
    Spectrogram
    WBP2600~3300 2600 3300 ／ 2850~3000 / ≥85 Φ0.1~300 Ge 400~10000
    Spectrogram
    WBP2600~5000 2490 5240 2640~5040 / ≥90 Φ0.1~300 Ge 400~7040
    Spectrogram
    WBP2650~3000 2650 3000 2700~2950 / ≥85 Φ0.1~300 Ge 1000~6000
    Spectrogram
    WBP2650~5050 2600 5050 2750~4950 / ≥90 Φ0.1~300 Kuma 1500~8000
    Spectrogram
    WBP2700~3150 2700 3150 ／ 2800~3050 / ≥80 Φ0.1~300 Ge 1500~5000
    Spectrogram
    WBP2700~2950 2700 2950 ／ 2750~2900 / ≥85 Φ0.1~300 Kuma 1500~6500
    Spectrogram
    WBP2700-3550 2700 3550 ／ 2800~3450 / ≥90 Φ0.1~300 Saffir 300~20000
    Spectrogram
    WBP2700-3600 2700 3600 ／ 2800~3500 / ≥90 Φ0.1~300 Saffir 300~20000
    Spectrogram
    WBP2720~2980 2720 2980 ／ 2780~2920 / ≥80 Φ0.1~300 Ge 1500~5000
    Spectrogram
    WBP2730~3010 2730 3010 ／ 2800~2900 / ≥85 Φ0.1~300 Ge 1500~5000
    Spectrogram
    WBP2750~4850 2750 4850 3000~4600 / ≥85 Φ0.1~300 Ge 1000~5100
    Spectrogram
    WBP2750~2950 2750 2950 ／ 2800~2900 / ≥85 Φ0.1~300 Kuma 1500~6500
    Spectrogram
    WBP2750~5100 2750 5100 2900~5000 / ≥90 Φ0.1~300 Ge 1500~10500
    Spectrogram
    WBP2790~3070 2790 3070 ／ 2900~3000 / ≥80 Φ0.1~300 Ge 1500~5000
    Spectrogram
    WBP2800~3050 2800 3050 ／ 2900~3000 / ≥90 Φ0.1~300 Kuma 1500~6500
    Spectrogram
    WBP2800~5150 2800 5150 ／ 2950~5000 / ≥90 Φ0.1~300 Ge 1500~10500
    Spectrogram
    WBP2800~5200 2800 5200 ／ 2950~5050 / ≥90 Φ0.1~300 Ge 1500~10500
    Spectrogram
    WBP 2800~5200 raka'a 2800 5200 2900~5100 ≥55 Φ0.1~300 Kuma 2580~8000
    Spectrogram
    WBP2800~5250 2800 5250 2950~5100 / ≥90 Φ0.1~300 Ge 1500~10500
    Spectrogram
    WBP2850~4150 3000~4000 / ≥90 Φ0.1~300 Saffir 400~11000
    Spectrogram
    WBP2850~5150 2850 5150 ／ 3000~5000 / ≥85 Φ0.1~300 Ge 1500~10500
    Spectrogram
    WBP2900~4140 2900 4140 ／ 3100~4040 / ≥90 Φ0.1~300 Ge 700~8040
    Spectrogram
    WBP2900~4450 2900 4450 3050~4350 / ≥85 Φ0.1~300 Ge 1500~10000
    Spectrogram
    WBP2900~4550 2900 4550 3050~4450 / ≥85 Φ0.1~300 Ge 1500~10000
    Spectrogram
    WBP2900~4850 2900 4850 3050~4750 / ≥90 Φ0.1~300 Kuma 400~11000
    Spectrogram
    WBP2900~4900 2800 3750 2900~3500 / ≥90 Φ0.1~300 Saffir 190~5500
    Spectrogram
    WBP2900~5100 2900 5100 ／ 3000~5000 / ≥90 Φ0.1~300 Ge 1000~10500
    Spectrogram
    WBP2950~3600 2950 3600 ／ 3150~3400 / ≥85 Φ0.1~300 Ge 1000~10500
    Spectrogram
    WBP2950~3650 2950 3650 ／ 3150~3450 / ≥85 Φ0.1~300 Ge 1000~10500
    Spectrogram
    WBP2950~3250 2950 3250 ／ 3000~3200 / ≥85 Φ0.1~300 Saffir 200~20000
    Spectrogram
    WBP2950~4950 2950 4950 3100~4800 / ≥90 Φ0.1~300 Kuma 400~11000
    Spectrogram
    WBP2950~5250 3000 5400 ／ 3100~5300 / ≥85 Φ0.1~300 Ge 1500~7000
    Spectrogram
    WBP3000~3300 3000 3300 ／ 3050~3250 / ≥85 Φ0.1~300 Saffir 200~20000
    Spectrogram
    WBP3000~3500 / / 480 3050~3400 / ≥80 Φ0.1~300 Quartz 300~6500
    Spectrogram
    WBP3000~3700 3000 3700 3100~3600 / ≥90 Φ0.1~300 Ge 200~10000
    Spectrogram
    WBP3000~3800 3000 3800 ／ 3100~3700 / ≥80 Φ0.1~300 Saffir 400~14000
    Spectrogram
    WBP3000~3875 3000 3875 ／ 3250~3650 / ≥80 Φ0.1~300 Saffir 500~5500
    Spectrogram
    WBP3000~4260 3000 4260 3250~3900 / ≥80 Φ0.1~300 Kuma 400~11000
    Spectrogram
    WBP3000~4300 3000 4300 3250~3900 / ≥80 Φ0.1~300 Kuma 400~11000
    Spectrogram
    WBP3000~5000 3000 5000 ／ 3100~4900 / ≥85 Φ0.1~300 Kuma 1500~11000
    Spectrogram
    WBP3000~5300 3000 5300 ／ 3150~5150 / ≥85 Φ0.1~300 Saffir 1500~15500
    Spectrogram
    WBP3000~5400 3000 5400 3100~5300 / ≥90 Φ0.1~300 Ge 1500~2800
    Spectrogram
    WBP3020~3320 3020 3320 3050~3250 / ≥85 Φ0.1~300 Saffir 200~20000
    Spectrogram
    WBP3040~4320 3040 4320 3250~4050 / ≥85 Φ0.1~300 Kuma 400~11000
    Spectrogram
    WBP3050~4200 3050 4200 3250~3900 / ≥85 Φ0.1~300 Kuma 400~11000
    Spectrogram
    WBP3050~5450 3050 5450 ／ 3200~5300 / ≥85 Φ0.1~300 Saffir 1500~15500
    Spectrogram
    WBP3050~5000 3050 5000 ／ 3200~4850 / ≥85 Φ0.1~300 Kuma 1500~10000
    Spectrogram
    WBP3100~3700 3100 3700 3200~3600 / ≥90 Φ0.1~300 Saffir 400~20000
    Spectrogram
    WBP3100~4100 3100 4100 3300~3900 / ≥90 Φ0.1~300 Ge 900~8000
    Spectrogram
    WBP3100~4150 3100 4150 ／ 3250~4050 / ≥90 Φ0.1~300 Ge 1500~10600
    Spectrogram
    1234567
    Jerin da ke sama yana nuna kayayyakin da muke da su a yanzu.
    Idan ba ka ga abin da kake nema ba, don Allah tuntuɓe mu.
    Tambayoyin da Ake Yawan Yi (FAQ)
    Q1: Me ake amfani da matatun Wide Bandpass (WBP)?
    An ƙera matatun mai faɗi da yawa don watsa haske mai faɗi yayin da suke toshe raƙuman ruwa da ba a so a wajen na'urar wucewa. Ana amfani da su sosai a cikin hotunan infrared, nazarin iskar gas, nazarin spectroscopy, da aikace-aikacen sa ido kan muhalli.
    Q2: Waɗanne kayan substrate ne ake da su don waɗannan matatun gani?
    Dangane da kewayon tsawon raƙuman da kake son amfani da su, muna bayar da matatun da aka ƙera a kan Sapphire, Silicon (Si), Germanium (Ge), Zinc Selenide (ZnSe), Quartz, da Glass Ceramics don tabbatar da ingantaccen watsawa da dorewa.
    Q3: Zan iya neman girma ko siffa ta musamman don matattarar ta?
    Eh, ƙarfin girman masana'anta na yau da kullun yana daga Φ0.1 mm har zuwa 300 mm. Za mu iya keɓance girma, siffofi, da bayanan gefe (gami da substrates masu siffar wedge) don dacewa da takamaiman tsarin kayan aikin ku.
    Q4: Menene yawan watsawa (Tavg) da kuma aikin toshewa?
    Yawancin matatunmu na kayanmu suna da matsakaicin matakan watsawa (Tavg) na ≥80% ko ≥90% a yankin da ke da cikakken haske, tare da aikin toshewa mai zurfi yana iyakance watsawa daga waje zuwa ƙasa da 1% (
    Q5: Ta yaya zan zaɓi tsakanin silicon (Si) da Germanium (Ge) substrates?
    Yawanci ana fifita silicon don kewayon infrared na 1.5 µm zuwa 6 µm kusa da tsakiyar saboda sauƙin nauyinsa da ƙarancin farashi. Germanium ya dace da aikace-aikacen infrared mai tsawo (har zuwa 12 µm da sama) da muhallin da ke buƙatar babban ma'aunin refractive.
    T6: Me zan yi idan wani takamaiman bayani bai bayyana a cikin kayanka ba?
    Idan kuna buƙatar takamaiman bayanai na gani na musamman, danna hanyar haɗin "tuntuɓe mu" don tuntuɓar ƙungiyar injiniyanmu. Muna ba da ƙira na musamman na rufin siriri da ƙera substrate don biyan buƙatun aikinku na musamman.

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