Title of article
The 16-day waves in the mesosphere and lower thermosphere over Wuhan (30.6°N, 114.5°E) and Adelaide (35°S, 138°E) Original Research Article
Author/Authors
Guo-ying Jiang، نويسنده , , Jian-Gang Xiong، نويسنده , , Weixing Wan، نويسنده , , Bai-Qi Ning، نويسنده , , Li-Bo Liu، نويسنده , , R.A. Vincent، نويسنده , , I. Reid، نويسنده ,
Issue Information
دوهفته نامه با شماره پیاپی سال 2005
Pages
6
From page
2005
To page
2010
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
Planetary wave , Mesosphere and lower thermosphere , 16-day waves
Journal title
Advances in Space Research
Serial Year
2005
Journal title
Advances in Space Research
Record number
1130234
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