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Ruled gratings

Ruled gratings

Ruled gratings are optical components used to separate light into its component wavelengths. Diffraction Gratings are used in spectroscopy, or for integration into spectrophotometers or monochromators.

Ruled gratings consist of a series of closely packed grooves that have been engraved or etched into the Grating’s surface. 

Product Details

Diffraction Ruled gratings are used in a variety of monochromators for research, student, and industry use. Almost all commercially available spectrophotometers (ultraviolet, visible, infrared, fluorescence, Raman, atomic absorption) utilize diffraction gratings to select specific wavelengths or scan over a wavelength interval. 

As a general rule, replicated Ruled gratings should be used when high peak efficiency and throughput are required. Replicated holographic gratings should be used when minimum stray light is critical and high resolution is needed. Note: Damage thresholds for both ruled and holographic gratings are 350 milli-joules/cm2 for pulsed lasers and 40 Watts/cm2 for CW lasers.

Ruled gratings  general specifications

Grooves20~1800Lines/mm
Blaze Wavelength250-10000nm
Blaze Angle4.3°-52.7°
Spectrum Length Coating19-26mm
CoatingAluminun
TypeReflective diffraction gratings
ConstructionRuled gratings

Ruled gratings catalogue 

ItemGroove(l/mm)Blaze WaveLeng(nm)Blaze AngleDimensions(mm)
GR10120100005.7°70*90
GR10220100005.7°63*105
GR103501280018.7°40*40
GR104501800026.7°60*63
GR105501060015.4°65*100
GR1067520004.3°48*48
GR10710025007.2°60*60
GR10810027507.9°64*64
GR109100700020.5°63*63
GR110100900026.7°20*20
GR111100980029.3°20*20
GR1121001060032°100*100
GR1131001600053.1°70*130
GR11415020008.6°55*60
GR115150400017.5°64*64
GR116150530023.4°25*25
GR117150600026.7°64*64
GR1181501000048.6°70*130
GR1191501060052.7°50*50
GR12020015508.9°38*41
GR121200180010.4°63*100
GR122200500030°55*55
GR1232508005.7°64*64
GR1243005004.3°64*64
GR1253006005.2°100*100
GR1263006405.5°64*64
GR12730010008.6°64*64
GR128300150013°64*64
GR129300190016.6°64*64
GR130300200017.5°64*64
GR131300240021.1°60*60
GR132300250022°64*64
GR133300275024.4°64*64
GR134300280024.8°50*50
GR135300300028.7°50*50
GR136300350032.7°50*50
GR137300380034.8°50*50
GR138300400035.9°50*50
GR139300500046.6°55*55
GR1404004304.9°35*50
GR1414005005.7°50*50
GR1424005406.2°48*50
GR143400150017.5°64*64
GR144400200023.6°64*64
GR1454504305.6°40*48
GR1466002504.3°64*64
GR1476003606.2°50*50
GR1486004307.4°40*40
GR1496005008.6°55*64
GR1506005409.3°85*85
GR15160060010.4°64*64
GR15260063010.9°17*44
GR15360064011.1°70*70
GR15460070012.1°64*64
GR15560072012.5°25*25
GR15660080013.9°20*45
GR157600100017.5°40*65
GR158600106018.5°40*65
GR159600125022°64*64
GR160600150026.7°64*64
GR161600160028.7°64*64
GR162600270054.1°20*90
GR16312002107.2°64*64
GR16412002508.6°64*64
GR165120031010.7°64*64
GR166120036012.5°55*55
GR167120043015°53*62
GR168120050017.5°102*102
GR169120054018.9°70*70
GR170120064022.6°100*102
GR171120072025.6°50*60
GR172120080028.7°50*100
GR1731200100036.9°50*60
GR1741200106039.5°100*105
GR175180021010.9°64*64
GR176180050026.7°50*50
GR177180050026.7°30*70
GR178180054029.1°30*70
GR179180072040.4°30*70