Earth Planets Space, 51, 621–628, 1999 Spatial structure of the 12-hour wave in the Antarctic as observed by radar

We present radar measurements of the 12-hour wave, a zonal wavenumber 1 westward propagating wave that exists in the southern polar mesopause region winds (Hernandez et al., 1993; Forbes et al., 1995). MF radar measurements of the horizontal winds at McMurdo (77.8◦S, 166.67◦E) show that the 12-hour...

Full description

Bibliographic Details
Main Authors: D. M. Riggin, D. C. Fritts, M. J. Jarvis, G. O. L. Jones
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Published: 1998
Subjects:
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.536.9851
http://www.terrapub.co.jp/journals/EPS/pdf/5107_08/51070621.pdf
id ftciteseerx:oai:CiteSeerX.psu:10.1.1.536.9851
record_format openpolar
spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.536.9851 2023-05-15T14:00:20+02:00 Earth Planets Space, 51, 621–628, 1999 Spatial structure of the 12-hour wave in the Antarctic as observed by radar D. M. Riggin D. C. Fritts M. J. Jarvis G. O. L. Jones The Pennsylvania State University CiteSeerX Archives 1998 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.536.9851 http://www.terrapub.co.jp/journals/EPS/pdf/5107_08/51070621.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.536.9851 http://www.terrapub.co.jp/journals/EPS/pdf/5107_08/51070621.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://www.terrapub.co.jp/journals/EPS/pdf/5107_08/51070621.pdf text 1998 ftciteseerx 2016-01-08T10:51:49Z We present radar measurements of the 12-hour wave, a zonal wavenumber 1 westward propagating wave that exists in the southern polar mesopause region winds (Hernandez et al., 1993; Forbes et al., 1995). MF radar measurements of the horizontal winds at McMurdo (77.8◦S, 166.67◦E) show that the 12-hour wave is highly seasonal, occurring during the austral summer solstice. During these seasonal occurrences, the wave is highly intermittent with amplitude peaks of>∼30 m s−1. The burst-like occurrences of large 12-hour wave amplitudes are highly correlated between the zonal and meridional direction. The diurnal tide over McMurdo has a more constant amplitude, but it is also an almost exclusively summertime phenomenon. Inertia-gravity wave activity is evident at periods less than 12 hr during the austral winter months. The weakening of gravity wave activity during the summer is probably due to critical layer filtering by the zonal mean wind, 12-hour wave and diurnal tide which are all strong during this season. The 12-hour wave is confined in height to the vicinity of the zero crossing in the zonal winds above the westward jet. Extreme distortion is observed in the vertical phase fronts of the 12-hour wave which could signify either refraction or in situ forcing. The distortion in the phase fronts and localization of the 12-hour wave in time and height is apparently responsible for departures in period from the nominal 12 hours. We do not find the wave period to be systematically different from 12 hours. The association of the 12-hour wave events with shear in the mean wind suggests that refractive effects could conceivably cause a dilation in wave amplitude. However, the shear is of the Text Antarc* Antarctic Unknown Antarctic Austral Forbes ENVELOPE(-66.550,-66.550,-67.783,-67.783) Hernandez ENVELOPE(-62.167,-62.167,-74.500,-74.500) The Antarctic
institution Open Polar
collection Unknown
op_collection_id ftciteseerx
language English
description We present radar measurements of the 12-hour wave, a zonal wavenumber 1 westward propagating wave that exists in the southern polar mesopause region winds (Hernandez et al., 1993; Forbes et al., 1995). MF radar measurements of the horizontal winds at McMurdo (77.8◦S, 166.67◦E) show that the 12-hour wave is highly seasonal, occurring during the austral summer solstice. During these seasonal occurrences, the wave is highly intermittent with amplitude peaks of>∼30 m s−1. The burst-like occurrences of large 12-hour wave amplitudes are highly correlated between the zonal and meridional direction. The diurnal tide over McMurdo has a more constant amplitude, but it is also an almost exclusively summertime phenomenon. Inertia-gravity wave activity is evident at periods less than 12 hr during the austral winter months. The weakening of gravity wave activity during the summer is probably due to critical layer filtering by the zonal mean wind, 12-hour wave and diurnal tide which are all strong during this season. The 12-hour wave is confined in height to the vicinity of the zero crossing in the zonal winds above the westward jet. Extreme distortion is observed in the vertical phase fronts of the 12-hour wave which could signify either refraction or in situ forcing. The distortion in the phase fronts and localization of the 12-hour wave in time and height is apparently responsible for departures in period from the nominal 12 hours. We do not find the wave period to be systematically different from 12 hours. The association of the 12-hour wave events with shear in the mean wind suggests that refractive effects could conceivably cause a dilation in wave amplitude. However, the shear is of the
author2 The Pennsylvania State University CiteSeerX Archives
format Text
author D. M. Riggin
D. C. Fritts
M. J. Jarvis
G. O. L. Jones
spellingShingle D. M. Riggin
D. C. Fritts
M. J. Jarvis
G. O. L. Jones
Earth Planets Space, 51, 621–628, 1999 Spatial structure of the 12-hour wave in the Antarctic as observed by radar
author_facet D. M. Riggin
D. C. Fritts
M. J. Jarvis
G. O. L. Jones
author_sort D. M. Riggin
title Earth Planets Space, 51, 621–628, 1999 Spatial structure of the 12-hour wave in the Antarctic as observed by radar
title_short Earth Planets Space, 51, 621–628, 1999 Spatial structure of the 12-hour wave in the Antarctic as observed by radar
title_full Earth Planets Space, 51, 621–628, 1999 Spatial structure of the 12-hour wave in the Antarctic as observed by radar
title_fullStr Earth Planets Space, 51, 621–628, 1999 Spatial structure of the 12-hour wave in the Antarctic as observed by radar
title_full_unstemmed Earth Planets Space, 51, 621–628, 1999 Spatial structure of the 12-hour wave in the Antarctic as observed by radar
title_sort earth planets space, 51, 621–628, 1999 spatial structure of the 12-hour wave in the antarctic as observed by radar
publishDate 1998
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.536.9851
http://www.terrapub.co.jp/journals/EPS/pdf/5107_08/51070621.pdf
long_lat ENVELOPE(-66.550,-66.550,-67.783,-67.783)
ENVELOPE(-62.167,-62.167,-74.500,-74.500)
geographic Antarctic
Austral
Forbes
Hernandez
The Antarctic
geographic_facet Antarctic
Austral
Forbes
Hernandez
The Antarctic
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_source http://www.terrapub.co.jp/journals/EPS/pdf/5107_08/51070621.pdf
op_relation http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.536.9851
http://www.terrapub.co.jp/journals/EPS/pdf/5107_08/51070621.pdf
op_rights Metadata may be used without restrictions as long as the oai identifier remains attached to it.
_version_ 1766269378990440448