Difference between revisions of "Optical Film Thickness & Wafer-Mapping (Filmetrics F50)"

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(pasted F20 text, update for F50)
 
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{{tool|{{PAGENAME}}
 
{{tool|{{PAGENAME}}
|picture=Filmmetrics_F50.jpg
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|picture=FIlmetrics_F50_Photo_v1.jpg
 
|type = Inspection, Test and Characterization
 
|type = Inspection, Test and Characterization
 
|super= Ning Cao
 
|super= Ning Cao
|phone=
 
 
|location=Bay 6
 
|location=Bay 6
|email=
 
 
|description = Thin-Film Reflectometry
 
|description = Thin-Film Reflectometry
 
|manufacturer = [http://www.filmetrics.com/ Filmetrics]
 
|manufacturer = [http://www.filmetrics.com/ Filmetrics]
|model = Filmetrics F50
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|model = F50
 
|materials =
 
|materials =
 
}}
 
}}
 
= About =
 
= About =
 
This tool is for thickness and optical property measurements of films on substrates, including mapping of thin-films on full wafers.
 
This tool is for thickness and optical property measurements of films on substrates, including mapping of thin-films on full wafers.
The technique used is white light reflection. Data is taken with normal incidence reflection of white light (190 nm – 1700 nm) from the surface using a Deuterium (UV) and Halogen (Vis-nIR) lamps. The motorized stage automatically acquires optical reflection spectra at programmed points across the wafer. The data is modeled at each point, and the optical parameters (thickness/refractive index/absorption) are adjusted to give a best least-squared fit to the data. The accuracy of the technique will depend on the thickness of the film and the optical models used for the fitting of the data. For a more complete description go to [http://www.filmetrics.com/ Filmetrics].
+
The technique used is white light reflection. Data is taken with normal incidence reflection of white light (190 nm – 1700 nm) from the surface using a Deuterium (UV) and Halogen (Vis-nIR) lamps.
  +
  +
The motorized stage automatically acquires optical reflection spectra at programmed points across the wafer. At each point, the reflection spectrum is baselines, and the reflection data is modeled at each point, and finally the optical parameters (thickness/refractive index/absorption) are adjusted to give a best least-squared fit to the data. The accuracy of the technique will depend on the thickness of the film and the optical models used for the fitting of the data. For a more complete description go to [http://www.filmetrics.com/ Filmetrics].
   
 
=Equipment Specifications=
 
=Equipment Specifications=
 
*190-1700 nm reflection spectrum
 
*190-1700 nm reflection spectrum
  +
*Deuterium (UV) and Halogen (Vis-nIR) light sources
*10 Å to 150 µm thickness, n, and k measurements
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*10 Å to 150 µm thickness, ''n'', and ''k'' measurements
*Accepts wafers up to 150mm for motorized mapping.
 
  +
*Motorized mapping on wafers up to 150mm.
 
*Small substrates also possible, ≥ 2-3mm
 
*Small substrates also possible, ≥ 2-3mm
*Data can be saved
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*Spectrum Data can be exported
 
*Can model up to three layers with accuracy
 
*Can model up to three layers with accuracy
  +
  +
=Operatin Procedures=
  +
''To be added''

Revision as of 15:10, 25 April 2019

Optical Film Thickness & Wafer-Mapping (Filmetrics F50)
FIlmetrics F50 Photo v1.jpg
Tool Type Inspection, Test and Characterization
Location Bay 6
Supervisor Ning Cao
Supervisor Phone (805) 893-4689
Supervisor E-Mail ningcao@ece.ucsb.edu
Description Thin-Film Reflectometry
Manufacturer Filmetrics
Model F50


About

This tool is for thickness and optical property measurements of films on substrates, including mapping of thin-films on full wafers. The technique used is white light reflection. Data is taken with normal incidence reflection of white light (190 nm – 1700 nm) from the surface using a Deuterium (UV) and Halogen (Vis-nIR) lamps.

The motorized stage automatically acquires optical reflection spectra at programmed points across the wafer. At each point, the reflection spectrum is baselines, and the reflection data is modeled at each point, and finally the optical parameters (thickness/refractive index/absorption) are adjusted to give a best least-squared fit to the data. The accuracy of the technique will depend on the thickness of the film and the optical models used for the fitting of the data. For a more complete description go to Filmetrics.

Equipment Specifications

  • 190-1700 nm reflection spectrum
  • Deuterium (UV) and Halogen (Vis-nIR) light sources
  • 10 Å to 150 µm thickness, n, and k measurements
  • Motorized mapping on wafers up to 150mm.
  • Small substrates also possible, ≥ 2-3mm
  • Spectrum Data can be exported
  • Can model up to three layers with accuracy

Operatin Procedures

To be added