Intradiurnal wind variations observed in the lower thermosphere over the

Abstract. The first meteor radar measurements of me-ridional winds in the lower thermosphere (about 95 5 km), along four azimuth directions: 0°, 90°E, 180 ° and 90°W; approximately 2 ° from the geographic South Pole were made during two observational cam-paigns: January 19, 1995–January 26, 1996, an...

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Main Authors: South Pole, Y. I. Portnyagin, J. M. Forbes, E. G. Merzlyakov, N. A. Makarov, S. E. Palo
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=10.1.1.590.8304
http://www.ann-geophys.net/18/547/2000/angeo-18-547-2000.pdf
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spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.590.8304 2023-05-15T18:22:08+02:00 Intradiurnal wind variations observed in the lower thermosphere over the South Pole Y. I. Portnyagin J. M. Forbes E. G. Merzlyakov N. A. Makarov S. E. Palo The Pennsylvania State University CiteSeerX Archives 1998 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.590.8304 http://www.ann-geophys.net/18/547/2000/angeo-18-547-2000.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.590.8304 http://www.ann-geophys.net/18/547/2000/angeo-18-547-2000.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://www.ann-geophys.net/18/547/2000/angeo-18-547-2000.pdf waves and text 1998 ftciteseerx 2016-01-08T13:31:03Z Abstract. The first meteor radar measurements of me-ridional winds in the lower thermosphere (about 95 5 km), along four azimuth directions: 0°, 90°E, 180 ° and 90°W; approximately 2 ° from the geographic South Pole were made during two observational cam-paigns: January 19, 1995–January 26, 1996, and No-vember 21, 1996–January 27, 1997. Herein we report analyses of the measurement results, obtained during the first campaign, which cover the whole one-year period, with particular emphasis on the transient nature and seasonal behavior of the main parameters of the intradiurnal wind oscillations. To analyze the data, two complementary methods are used: the well-known periodogram (FFT) technique and the S-transform technique. The most characteristic periods of the intra-diurnal oscillations are found to be rather uniformly spread between about 7 h and 12 h. All of these oscillations are westward-propagating with zonal wave number s 1 and their usual duration is confined to several periods. During the austral winter season the oscillations with periods less than 12 h are the most intensive, while during summer season the 12-h oscilla-tions dominate. Lamb waves and internal-gravity wave propagation, non-linear interaction of the short-period tides, excitation in situ of the short period waves may be considered as possible processes which are responsible for intradiurnal wind oscillations in the lower thermo-sphere over South Pole. Key words: Meteorology and atmospheric dynamics (middle atmosphere dynamics; thermospheric dynamics; Text South pole Unknown Austral South Pole
institution Open Polar
collection Unknown
op_collection_id ftciteseerx
language English
topic waves and
spellingShingle waves and
South Pole
Y. I. Portnyagin
J. M. Forbes
E. G. Merzlyakov
N. A. Makarov
S. E. Palo
Intradiurnal wind variations observed in the lower thermosphere over the
topic_facet waves and
description Abstract. The first meteor radar measurements of me-ridional winds in the lower thermosphere (about 95 5 km), along four azimuth directions: 0°, 90°E, 180 ° and 90°W; approximately 2 ° from the geographic South Pole were made during two observational cam-paigns: January 19, 1995–January 26, 1996, and No-vember 21, 1996–January 27, 1997. Herein we report analyses of the measurement results, obtained during the first campaign, which cover the whole one-year period, with particular emphasis on the transient nature and seasonal behavior of the main parameters of the intradiurnal wind oscillations. To analyze the data, two complementary methods are used: the well-known periodogram (FFT) technique and the S-transform technique. The most characteristic periods of the intra-diurnal oscillations are found to be rather uniformly spread between about 7 h and 12 h. All of these oscillations are westward-propagating with zonal wave number s 1 and their usual duration is confined to several periods. During the austral winter season the oscillations with periods less than 12 h are the most intensive, while during summer season the 12-h oscilla-tions dominate. Lamb waves and internal-gravity wave propagation, non-linear interaction of the short-period tides, excitation in situ of the short period waves may be considered as possible processes which are responsible for intradiurnal wind oscillations in the lower thermo-sphere over South Pole. Key words: Meteorology and atmospheric dynamics (middle atmosphere dynamics; thermospheric dynamics;
author2 The Pennsylvania State University CiteSeerX Archives
format Text
author South Pole
Y. I. Portnyagin
J. M. Forbes
E. G. Merzlyakov
N. A. Makarov
S. E. Palo
author_facet South Pole
Y. I. Portnyagin
J. M. Forbes
E. G. Merzlyakov
N. A. Makarov
S. E. Palo
author_sort South Pole
title Intradiurnal wind variations observed in the lower thermosphere over the
title_short Intradiurnal wind variations observed in the lower thermosphere over the
title_full Intradiurnal wind variations observed in the lower thermosphere over the
title_fullStr Intradiurnal wind variations observed in the lower thermosphere over the
title_full_unstemmed Intradiurnal wind variations observed in the lower thermosphere over the
title_sort intradiurnal wind variations observed in the lower thermosphere over the
publishDate 1998
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.590.8304
http://www.ann-geophys.net/18/547/2000/angeo-18-547-2000.pdf
geographic Austral
South Pole
geographic_facet Austral
South Pole
genre South pole
genre_facet South pole
op_source http://www.ann-geophys.net/18/547/2000/angeo-18-547-2000.pdf
op_relation http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.590.8304
http://www.ann-geophys.net/18/547/2000/angeo-18-547-2000.pdf
op_rights Metadata may be used without restrictions as long as the oai identifier remains attached to it.
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