Characterization of exceptionally strong mesospheric wave events using all-sky and zenith airglow observations

Two unusually clear mesospheric gravity wave events were observed by the Boston University all-sky imager and the Argentine airglow spectrometer on two consecutive nights at the El Leoncito Observatory, Argentina (31.8°S, 69.3°W), during August 2001. Both events exhibited brightness amplitudes an or...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Smith, S.M., Scheer, J., Reisin, E.R., Baumgardner, J., Mendillo, M.
Formato: JOUR
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_21699402_v111_n9_p_Smith
Aporte de:
id todo:paper_21699402_v111_n9_p_Smith
record_format dspace
spelling todo:paper_21699402_v111_n9_p_Smith2023-10-03T16:40:07Z Characterization of exceptionally strong mesospheric wave events using all-sky and zenith airglow observations Smith, S.M. Scheer, J. Reisin, E.R. Baumgardner, J. Mendillo, M. Two unusually clear mesospheric gravity wave events were observed by the Boston University all-sky imager and the Argentine airglow spectrometer on two consecutive nights at the El Leoncito Observatory, Argentina (31.8°S, 69.3°W), during August 2001. Both events exhibited brightness amplitudes an order of magnitude above typical values. The first event had the appearance of a large-amplitude (>60% in OH(6-2), 22% in O 2 , and 37% in O( 1 S) emissions (peak to peak), compared to 1-5% typically), upward propagating gravity wave with pronounced nonlinear behavior. The waves also showed noticeably curved wavefronts, indicating that they had originated from a relatively small source region within ∼180 km of El Leoncito. Estimates of the vertical flux of horizontal energy and momentum for the wave event in the OH and O 2 emissions were very large compared to typical values, and they also indicated a high degree of flux divergence over the nominal 8 km altitude between the two layers. The second event occurred on the following night and exhibited a frontal morphology and behavior consistent with an internal ducted gravity wave showing nonlinear behavior akin to a mesospheric bore. The disturbance also had several interesting characteristics; in particular, the propagation speed decreased during its passage across the sky. In addition, a strong vertical temperature gradient due to the semidiurnal tide appeared to influence the occurrence of the bore event. Copyright 2006 by the American Geophysical Union. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_21699402_v111_n9_p_Smith
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description Two unusually clear mesospheric gravity wave events were observed by the Boston University all-sky imager and the Argentine airglow spectrometer on two consecutive nights at the El Leoncito Observatory, Argentina (31.8°S, 69.3°W), during August 2001. Both events exhibited brightness amplitudes an order of magnitude above typical values. The first event had the appearance of a large-amplitude (>60% in OH(6-2), 22% in O 2 , and 37% in O( 1 S) emissions (peak to peak), compared to 1-5% typically), upward propagating gravity wave with pronounced nonlinear behavior. The waves also showed noticeably curved wavefronts, indicating that they had originated from a relatively small source region within ∼180 km of El Leoncito. Estimates of the vertical flux of horizontal energy and momentum for the wave event in the OH and O 2 emissions were very large compared to typical values, and they also indicated a high degree of flux divergence over the nominal 8 km altitude between the two layers. The second event occurred on the following night and exhibited a frontal morphology and behavior consistent with an internal ducted gravity wave showing nonlinear behavior akin to a mesospheric bore. The disturbance also had several interesting characteristics; in particular, the propagation speed decreased during its passage across the sky. In addition, a strong vertical temperature gradient due to the semidiurnal tide appeared to influence the occurrence of the bore event. Copyright 2006 by the American Geophysical Union.
format JOUR
author Smith, S.M.
Scheer, J.
Reisin, E.R.
Baumgardner, J.
Mendillo, M.
spellingShingle Smith, S.M.
Scheer, J.
Reisin, E.R.
Baumgardner, J.
Mendillo, M.
Characterization of exceptionally strong mesospheric wave events using all-sky and zenith airglow observations
author_facet Smith, S.M.
Scheer, J.
Reisin, E.R.
Baumgardner, J.
Mendillo, M.
author_sort Smith, S.M.
title Characterization of exceptionally strong mesospheric wave events using all-sky and zenith airglow observations
title_short Characterization of exceptionally strong mesospheric wave events using all-sky and zenith airglow observations
title_full Characterization of exceptionally strong mesospheric wave events using all-sky and zenith airglow observations
title_fullStr Characterization of exceptionally strong mesospheric wave events using all-sky and zenith airglow observations
title_full_unstemmed Characterization of exceptionally strong mesospheric wave events using all-sky and zenith airglow observations
title_sort characterization of exceptionally strong mesospheric wave events using all-sky and zenith airglow observations
url http://hdl.handle.net/20.500.12110/paper_21699402_v111_n9_p_Smith
work_keys_str_mv AT smithsm characterizationofexceptionallystrongmesosphericwaveeventsusingallskyandzenithairglowobservations
AT scheerj characterizationofexceptionallystrongmesosphericwaveeventsusingallskyandzenithairglowobservations
AT reisiner characterizationofexceptionallystrongmesosphericwaveeventsusingallskyandzenithairglowobservations
AT baumgardnerj characterizationofexceptionallystrongmesosphericwaveeventsusingallskyandzenithairglowobservations
AT mendillom characterizationofexceptionallystrongmesosphericwaveeventsusingallskyandzenithairglowobservations
_version_ 1807317153239531520