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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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 |
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waves and |
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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. |
_version_ |
1766201488472801280 |