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

• Main Authors: Alam, Omar B. (Author), Noto, John (Author), Kerr, Robert B. (Author), Kapali, Sudha (Author), Rogers, Alan E E (Contributor), Erickson, Philip J (Contributor), Goncharenko, Larisa (Contributor)
• Other Authors: Haystack Observatory (Contributor)
• Format: Article
• Language: English
• Published: American Meteorological Society, 2017-03-23T17:18:33Z.
• Subjects: Article
• Online Access: Get fulltext

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.
National Science Foundation (U.S.) Research Experiences for Undergraduates (Grant AST-1156504)