Open AccessEvidence of reflection of a long‐period gravity wave in observations of the nightglow over Arecibo on May 8–9, 1989
Author(s) -
Walterscheid R. L.,
Hecht J. H.,
Djuth F. T.,
Tepley C. A.
Publication year - 2000
Publication title -
journal of geophysical research: atmospheres
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/1999jd901065
Subject(s) - airglow , thermosphere , brightness , atmospheric sciences , atmosphere (unit) , wavelength , meteor (satellite) , phase (matter) , gravity wave , mesopause , reflection (computer programming) , physics , mesosphere , depth sounding , geology , ionosphere , geophysics , meteorology , optics , astronomy , gravitational wave , oceanography , quantum mechanics , computer science , programming language , stratosphere
During the Arecibo Initiative in Dynamics of the Atmosphere (AIDA) campaign there were several unusual observations of the O 2 Atmospheric (0,1) and OH Meinel (6,2) brightness fluctuations being nearly 180° out of phase. In this paper we discuss data from May 8–9, 1989, during which meteor radar and airglow instrumentations were operating and thus wind data were available. We show that the nearly out‐of‐phase result on this night is due to the fact that the OH Meinel brightness and temperature are out of phase while the O 2 atmospheric temperature and brightness are nearly in phase. The characteristics of the wave causing the out of phase fluctuations are derived and comparisons are made between results obtained by the Aerospace nightglow camera and those obtained by the York University airglow camera [ Zhang et al ., 1993]. Although there are differences between them, both of the instrumental data sets are consistent with the presence of a wave with a horizontal wavelength ≥600 km and a period of several hours. An analysis of these data shows that the out‐of‐phase relationship is most likely due to strong wave reflection in the lower thermosphere caused by thermal gradients and wind shears.