Home Contact Us catalog price list Order Info

cap space products space services space technical space applications space corporate space distributors space cap

technical
operating instructions
software downloads
Engineering Docs
system specifications
patent informaiton
discontinued products
video tutorials

 
Google Custom Search
 
Get our eNewswire
Email:  
 

 

 

 

Optical Resolution 

Optical resolution of a monochromatic source -- -- measured as Full Width Half Maximum (FWHM) -- depends on the groove density (mm-1) of the grating and the diameter of the entrance optics (optical fiber or slit). In configuring your spectrometer, consider two important trade-offs:

1) Resolution increases with an increase in the groove density of the grating, but at the expense of spectral range and signal strength; and

2) Resolution increases as the slit width or fiber diameter decreases, but at the expense of signal strength.

How to Calculate the Approximate Optical Resolution in nm (FWHM)

1. Determine the Spectral Range of the Grating. You can find the Spectral Range of Gratings at:

2. Divide the Spectral Range of the Grating by the Number of Detector Elements. The resulting value is the Dispersion.

Dispersion (nm/pixel) = Spectral Range of the Grating/Number of Detector Elements

The table below lists the Detector Elements for various spectrometer benches and models.

Spectrometer Number of Detector Elements
USB2000 Spectrometer 2048
USB4000 Spectrometer 3648
HR2000 Spectrometer 2048
HR4000 Spectrometer 3648
NIR256-2.1 Spectrometer 256
NIR256-2.5 Spectrometer 256
NIR512 Spectrometer 512
QE65000 Spectrometer 1044

3. Determine the Pixel Resolution

The pixel resolution is listed below for various sizes of slits (or the optical fiber diameter if the fiber is the limiting factor). The width of the Entrance Aperture Slits differ; the Height of all slits are the same (1000 microns).

  5 micron
Slit
10 micron
Slit
25 micron
Slit
50 micron
Slit
100 micron
Slit
200 micron
Slit
USB2000 Spectrometer ~3.0 pixels ~3.2 pixels ~4.2 pixels ~6.5 pixels ~12.0 pixels ~24.0 pixels
USB4000 Spectrometer ~5.3 pixels ~5.7 pixels ~7.5 pixels ~11.6 pixels ~21.0 pixels ~42.0 pixels
HR2000 Spectrometer ~1.5 pixels ~2.0 pixels ~2.5 pixels ~4.2 pixels ~8.0 pixels ~15.3 pixels
HR2000+ Spectrometer ~1.5 pixels ~2.0 pixels ~2.5 pixels ~4.2 pixels ~8.0 pixels ~15.3 pixels
HR4000 Spectrometer ~2.0 pixels ~3.7 pixels ~4.4 pixels ~7.4 pixels ~14.0 pixels ~26.8 pixels
NIR256-2.1 Spectrometer N/A ~1.2 pixels ~1.2 pixels ~1.5 pixels ~2.2 pixels ~4.0 pixels
NIR256-2.5 Spectrometer N/A ~1.2 pixels ~1.2 pixels ~1.5 pixels ~2.2 pixels ~4.0 pixels
NIR512 Spectrometer N/A ~2.4 pixels ~2.4 pixels ~2.9 pixels ~4.4 pixels ~7.9 pixels
QE65000 Spectrometer ~2.0 pixels ~2.2 pixels ~2.6 pixels ~3.3 pixels ~4.7 pixels ~8.9 pixels

4. Calculate the Optical Resolution (in nm)

Dispersion (Step 2) x Pixel Resolution (Step 3)

Example: Determine the Optical Resolution of a USB4000 Spectrometer with Grating #3, 10-micron Slit

650 nm (spectral range of Grating #3)/3648 (detector elements in USB4000) = 0.18 nm/pixel x 5.6 pixels = 1.0 nm (FWHM)

Note: Values rounded up to nearest tenth.

 

 

 

 

 


Contact an Ocean Optics Applications Scientist

  

System Sensitivity

 

Operating Principles