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Maintenance of zonal wind variability associated with the annular mode on Mars
Author(s) -
Yamashita Yousuke,
Kuroda Takeshi,
Takahashi Masaaki
Publication year - 2007
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2007gl030069
Subject(s) - baroclinity , empirical orthogonal functions , martian , forcing (mathematics) , barotropic fluid , mars exploration program , geology , atmospheric wave , atmosphere of mars , wavenumber , mode (computer interface) , transient (computer programming) , geophysics , physics , atmospheric sciences , mechanics , climatology , wave propagation , gravity wave , astrobiology , optics , quantum mechanics , computer science , operating system
Results from a Mars general circulation model (MGCM) were used to investigate the maintenance of the annular mode in the Martian atmosphere. Analysis of the Martian northern winter, as represented by the MGCM, revealed a prominent transient wave with zonal wave number 1 that had a baroclinic instability structure. An empirical orthogonal function (EOF) decomposition showed that the first two modes of the EOF contained features of the transient wave with wave number 1. The third EOF mode had an annular structure about the Martian North Pole and an equivalent barotropic structure in the vertical. Each term in the transformed Eulerian mean equation was estimated from the MGCM output to investigate the maintenance of the annular mode. Wave forcing (Eliassen‐Palm flux divergence) played an important role in maintaining the mode. In the wave forcing term, contributions from transient baroclinic waves with wave numbers 1 and 2 were important.