Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

Comparison of Ozone Columns between FTIR and CLAES over Mauna Loa, Hawaii

Not Accessible

Your library or personal account may give you access

Abstract

Very high resolution infrared solar spectra have been collected from Mauna Loa Observatory by a Fourier Transform Spectrometer (FTS) system. Observations have been made every Wednesday morning (weather permitting) since November, 1991, by the staff of the Observatory, which is operated by the Climate Monitoring and Diagnostics Laboratory of NOAA. The instrument currently covers two spectral regions: 800 to 1200 cm−1 and 2800 to 3200 cm−1. Many atmospheric gases have absorptions in these regions which can be used to recover abundance information. Both regions include absorptions due to ozone. For this study, regions near 1146 and 1163 cm−1 have been fitted to recover ozone columns.

© 1993 Optical Society of America

PDF Article
More Like This
NDSC Infrared Observations at Mauna Loa, Hawaii

F.J. Murcray, D.G. Murcray, S.J. David, R.D. Blatherwick, J.J. Kosters, F.H. Murcray, A. Goldman, and C.P. Rinsland
ThC.4 Optical Remote Sensing of the Atmosphere (ORS) 1993

High Resolution Infrared Solar Spectra from Mauna Loa Observatory

Shelle J. David and Frank J. Murcray
TuC6 Optical Remote Sensing of the Atmosphere (ORS) 1995

Lidar Measurements of Stratospheric Aerosols at Mauna Loa Observatory: 1974 to Present

T. E. DeFoor, S. Ryan, D. J. Hofmann, and E. G. Dutton
ThA.1 Optical Remote Sensing of the Atmosphere (ORS) 1993

Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.