Seasonal and Local Solar Time Variation of the Meridional Wind at 95 km from Observations of the 11.072-GHz Ozone Line and the 557.7-nm Oxygen Line
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Seasonal and Local Solar Time Variation.pdf
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1.19 MB
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Adobe PDF
Checksum (MD5)
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Author(s)
Alam, Omar B.
Noto, John
Kerr, Robert B.
Kapali, Sudha
Rogers, Alan E E
Erickson, Philip J
Goncharenko, Larisa
Date Issued
June 2016
Journal
Journal of Atmospheric and Oceanic Technology
Publisher
American Meteorological Society
Citation
Rogers, Alan E. E. et al. “Seasonal and Local Solar Time Variation of the Meridional Wind at 95 Km from Observations of the 11.072-GHz Ozone Line and the 557.7-Nm Oxygen Line.” Journal of Atmospheric and Oceanic Technology 33.7 (2016): 1355–1361. © 2016 American Meteorological Society
Version
Final published version
Abstract
Ground-based spectrometers have been deployed to measure the concentration, velocity, and temperature of ozone in the mesosphere and lower thermosphere (MLT), using low-cost satellite television electronics to observe the 11.072-GHz line of ozone. The ozone line was observed at an altitude near 95 km at 38°N, 71°W using three spectrometers located at the Massachusetts Institute of Technology’s Haystack Observatory (Westford, Massachusetts), Chelmsford High School (Chelmsford, Massachusetts), and Union College (Schenectady, New York), each pointed south at 8° elevation. Observations from 2009 through 2014 were used to derive the nightly averaged seasonal variation of the 95-km altitude meridional wind velocity, as well as the seasonally averaged variation of the meridional wind with local solar time. The results indicate a seasonal trend in which the winds at 95 km are directed southward at about 10 m s[superscript −1] in the summer of the Northern Hemisphere and northward at about 10 m s[superscript −1] in the winter. Nighttime data from −5 to +5 local solar time show a gradual transition of the meridional wind velocity from about −20 to 20 m s[superscript −1]. These variations correlate well with nighttime wind measurements using 557.7-nm optical airglow observations from the Millstone Hill high-resolution Fábry–Perot interferometer (FPI) in Westford.
MIT Department
Haystack Observatory
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DOI of Published Version
https://doi.org/10.1175/jtech-d-15-0247.1
