Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/39302
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Type: Journal article
Title: The 16-day waves in the mesosphere and lower thermosphere over Wuhan (30.6°N 114.5°E) and Adelaide (35°S 138°E)
Other Titles: The 16-day waves in the mesosphere and lower thermosphere over Wuhan (30.6 degrees N 114.5 degrees E) and Adelaide (35 degrees S 138 degrees E)
Author: Jiang, G.
Xiong, J.
Wan, W.
Ning, B.
Liu, L.
Vincent, R.
Reid, I.
Citation: Advances in Space Research, 2005; 35(11):2005-2010
Publisher: Pergamon-Elsevier Science Ltd
Issue Date: 2005
ISSN: 0273-1177
Editor: Clemesha, B.
Taylor, M.
Statement of
Responsibility: 
Guo-ying Jiang, Jian-Gang Xiong, Wei-Xing Wan, Bai-Qi Ning, Li-Bo Liu, R.A. Vincent and I. Reid
Abstract: Winds from a meteor radar at Wuhan (30.6°N, 114.5°E) and a MF radar at Adelaide (35°S, 138°E) are used to study the 16-day waves in the mesosphere and lower thermosphere (MLT). The height range is 78–98 km at Wuhan and 70–98 km at Adelaide. By comparison, it is found that the zonal components at both sites are generally larger than the meridional ones, and eastward motion of the zonal background winds is favorable for the 16-day waves penetration to the MLT region. The zonal maximum amplitude appears in the autumn (September–October) around 86–98 km at Wuhan and in the winter months and early spring (July–October) around 72–82 km at Adelaide. Differences are found in wave amplitudes and time of appearance between the two years of 2002 and 2003. In 2003, the intensity of the wave amplitudes is relatively smaller than that for 2002 at both sites. The summer 16-day waves are comparatively weaker at Adelaide in both years, but stronger in 2002 at Wuhan near the mesopause and the lower thermosphere (86–98 km). The strong summer waves at Wuhan may come from the winter southern hemisphere.
Keywords: 16-day waves
Mesosphere and lower thermosphere
Planetary wave
DOI: 10.1016/j.asr.2005.03.011
Description (link): http://www.elsevier.com/wps/find/journaldescription.cws_home/644/description#description
Published version: http://dx.doi.org/10.1016/j.asr.2005.03.011
Appears in Collections:Aurora harvest
Chemistry and Physics publications

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