Approach for obtaining best estimates of spectral optical depths and calibration intercepts from solar radiometer data corrupted by temporal variations

Wayne H. Erxleben, John A. Reagan

Research output: Contribution to conferencePaper

1 Scopus citations

Abstract

Calibration of solar radiometers is generally accomplished by the Langley plot method; however, slight temporal variations in optical depth can significantly bias zero-airmass intercepts thus derived. This paper presents signal processing techniques for improving the Langley analysis under temporally varying conditions, as well as better characterizing the variability itself. These techniques include spectral analysis of the data to identify systematic atmospheric variations and distinguish them from measurement noise, and exploitation of the correlation between measurements at different wavelengths and on different days. The processing is applied to data from an automated 10-channel radiometer.

Original languageEnglish (US)
Pages1014-1016
Number of pages3
StatePublished - Jan 1 1996
EventProceedings of the 1996 International Geoscience and Remote Sensing Symposium, IGARSS'96. Part 1 (of 4) - Lincoln, NE, USA
Duration: May 28 1996May 31 1996

Other

OtherProceedings of the 1996 International Geoscience and Remote Sensing Symposium, IGARSS'96. Part 1 (of 4)
CityLincoln, NE, USA
Period5/28/965/31/96

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ASJC Scopus subject areas

  • Computer Science Applications
  • Earth and Planetary Sciences(all)

Cite this

Erxleben, W. H., & Reagan, J. A. (1996). Approach for obtaining best estimates of spectral optical depths and calibration intercepts from solar radiometer data corrupted by temporal variations. 1014-1016. Paper presented at Proceedings of the 1996 International Geoscience and Remote Sensing Symposium, IGARSS'96. Part 1 (of 4), Lincoln, NE, USA, .