New Pyro-Optic techniques for Imaging of Long Wavelength IR-Radiation (Pyro-Optic Initiation Program)

Abstract

From a simple consideration of the thermal conversation efficiency which can be realized in the non contact pyro-optic system it is shown that for f/l optics a scene temperature change of 0. 1 deg C will realize a change at the detector of 0.001 deg C for a detector thickness of 0.1 micrometer, chopping frequency of 25 Hz. For a simple pixel element 50 micron x 50 micron x 0.1 micron the RMS thermal noise limit in SBSI is calculated to be 3.5 x 10 to the - 5 deg C well below the expected signal level. Using a very simple ellipsometric setup working into a photomultiplier detector it is shown that for SbSI single crystals and thin films, temperature oscillations of 0.001 deg C can be detected above noise level.

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Document Details

Document Type
Technical Report
Publication Date
Dec 21, 1992
Accession Number
ADA260969

Entities

People

  • A. S. Bhalla
  • Leslie Eric Cross

Organizations

  • Pennsylvania State University

Tags

Communities of Interest

  • Advanced Electronics
  • Energy and Power Technologies

DTIC Thesaurus Topics

  • Amplifiers
  • Climate Change
  • Crystals
  • Detection
  • Detectors
  • Efficiency
  • Films
  • Frequency
  • Long Wavelengths
  • Materials
  • Optical Detection
  • Optics
  • Radiation
  • Single Crystals
  • Specific Heat
  • Thickness
  • Thin Films

Fields of Study

  • Physics

Readers

  • Electronics Engineering
  • Spectroscopy.
  • Thin Film Deposition Science.