Articles | Volume 33, issue 11
https://doi.org/10.5194/angeo-33-1349-2015
https://doi.org/10.5194/angeo-33-1349-2015
Regular paper
 | 
06 Nov 2015
Regular paper |  | 06 Nov 2015

Interhemispheric structure and variability of the 5-day planetary wave from meteor radar wind measurements

H. Iimura, D. C. Fritts, D. Janches, W. Singer, and N. J. Mitchell

Viewed

Total article views: 1,713 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
901 744 68 1,713 74 74
  • HTML: 901
  • PDF: 744
  • XML: 68
  • Total: 1,713
  • BibTeX: 74
  • EndNote: 74
Views and downloads (calculated since 06 Nov 2015)
Cumulative views and downloads (calculated since 06 Nov 2015)

Cited

Latest update: 13 Dec 2024
Download
Short summary
The quasi-5-day wave at mid- and high-latitudes in the mesosphere and lower-thermosphere was compared between the hemispheres using meteor radar horizontal wind measurements, spanning June 2010 to December 2012. Variances of the quasi-5-day wave showed a wave activity from July to August in both hemispheres and in April 2012 in the Northern Hemisphere and November 2012 in the Southern Hemisphere with unique characteristics at each site.