Regional variations of mesospheric gravity-wave momentum flux over Antarctica
Images of mesospheric airglow and radar-wind measurements have been combined to estimate the difference in the vertical flux of horizontal momentum carried by high-frequency gravity waves over two dissimilar Antarctic stations. Rothera (67° S, 68° W) is situated in the mountains o...
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Copernicus Publications
2006-03-01
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Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/24/81/2006/angeo-24-81-2006.pdf |
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author | P. J. Espy R. E. Hibbins G. R. Swenson J. Tang M. J. Taylor D. M. Riggin D. C. Fritts |
author_facet | P. J. Espy R. E. Hibbins G. R. Swenson J. Tang M. J. Taylor D. M. Riggin D. C. Fritts |
author_sort | P. J. Espy |
collection | DOAJ |
description | Images of mesospheric airglow and radar-wind measurements have been combined
to estimate the difference in the vertical flux of horizontal momentum
carried by high-frequency gravity waves over two dissimilar Antarctic
stations. Rothera (67° S, 68° W) is situated in the mountains of the
Peninsula near the edge of the wintertime polar vortex. In contrast, Halley
(76° S, 27° W), some 1658 km to the southeast, is located on an ice
sheet at the edge of the Antarctic Plateau and deep within the polar vortex
during winter. The cross-correlation coefficients between the vertical and
horizontal wind perturbations were calculated from sodium (Na) airglow
imager data collected during the austral winter seasons of 2002 and 2003 at
Rothera for comparison with the 2000 and 2001 results from Halley reported
previously (Espy et al., 2004). These cross-correlation coefficients were combined with
wind-velocity variances from coincident radar measurements to estimate the
daily averaged upper-limit of the vertical flux of horizontal momentum due
to gravity waves near the peak emission altitude of the Na nightglow layer,
90km. The resulting momentum flux at both stations displayed a large
day-to-day variability and showed a marked seasonal rotation from the
northwest to the southwest throughout the winter. However, the magnitude of
the flux at Rothera was about 4 times larger than that at Halley, suggesting
that the differences in the gravity-wave source functions and filtering by
the underlying winds at the two stations create significant regional
differences in wave forcing on the scale of the station separation. |
first_indexed | 2024-12-20T22:33:02Z |
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id | doaj.art-f63124c7497d428b877a76b6a672ba9c |
institution | Directory Open Access Journal |
issn | 0992-7689 1432-0576 |
language | English |
last_indexed | 2024-12-20T22:33:02Z |
publishDate | 2006-03-01 |
publisher | Copernicus Publications |
record_format | Article |
series | Annales Geophysicae |
spelling | doaj.art-f63124c7497d428b877a76b6a672ba9c2022-12-21T19:24:41ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762006-03-0124818810.5194/angeo-24-81-2006Regional variations of mesospheric gravity-wave momentum flux over AntarcticaP. J. Espy0R. E. Hibbins1G. R. Swenson2J. Tang3M. J. Taylor4D. M. Riggin5D. C. Fritts6The British Antarctic Survey, NERC, Cambridge, UKThe British Antarctic Survey, NERC, Cambridge, UKDepartment of Electrical & Computer Engineering, University of Illinois at Urbana-Champaign, USADepartment of Electrical & Computer Engineering, University of Illinois at Urbana-Champaign, USADepartment of Physics, Utah State University, Logan, Utah, USAColorado Research Associates, a division of NorthWest Research Associates, Boulder, Colorado, USAColorado Research Associates, a division of NorthWest Research Associates, Boulder, Colorado, USAImages of mesospheric airglow and radar-wind measurements have been combined to estimate the difference in the vertical flux of horizontal momentum carried by high-frequency gravity waves over two dissimilar Antarctic stations. Rothera (67° S, 68° W) is situated in the mountains of the Peninsula near the edge of the wintertime polar vortex. In contrast, Halley (76° S, 27° W), some 1658 km to the southeast, is located on an ice sheet at the edge of the Antarctic Plateau and deep within the polar vortex during winter. The cross-correlation coefficients between the vertical and horizontal wind perturbations were calculated from sodium (Na) airglow imager data collected during the austral winter seasons of 2002 and 2003 at Rothera for comparison with the 2000 and 2001 results from Halley reported previously (Espy et al., 2004). These cross-correlation coefficients were combined with wind-velocity variances from coincident radar measurements to estimate the daily averaged upper-limit of the vertical flux of horizontal momentum due to gravity waves near the peak emission altitude of the Na nightglow layer, 90km. The resulting momentum flux at both stations displayed a large day-to-day variability and showed a marked seasonal rotation from the northwest to the southwest throughout the winter. However, the magnitude of the flux at Rothera was about 4 times larger than that at Halley, suggesting that the differences in the gravity-wave source functions and filtering by the underlying winds at the two stations create significant regional differences in wave forcing on the scale of the station separation.https://www.ann-geophys.net/24/81/2006/angeo-24-81-2006.pdf |
spellingShingle | P. J. Espy R. E. Hibbins G. R. Swenson J. Tang M. J. Taylor D. M. Riggin D. C. Fritts Regional variations of mesospheric gravity-wave momentum flux over Antarctica Annales Geophysicae |
title | Regional variations of mesospheric gravity-wave momentum flux over Antarctica |
title_full | Regional variations of mesospheric gravity-wave momentum flux over Antarctica |
title_fullStr | Regional variations of mesospheric gravity-wave momentum flux over Antarctica |
title_full_unstemmed | Regional variations of mesospheric gravity-wave momentum flux over Antarctica |
title_short | Regional variations of mesospheric gravity-wave momentum flux over Antarctica |
title_sort | regional variations of mesospheric gravity wave momentum flux over antarctica |
url | https://www.ann-geophys.net/24/81/2006/angeo-24-81-2006.pdf |
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