Diurnal Kelvin wave in the atmosphere of Mars: Towards an understanding of 'stationary' density structures observed by the MGS accelerometer

Forbes, M.; Hagan, E.

doi:10.1029/2000GL011850

Forbes, J. M., & Hagan, M. E. (2000). Diurnal Kelvin wave in the atmosphere of Mars: Towards an understanding of 'stationary' density structures observed by the MGS accelerometer. Geophysical Research Letters, 27, 3563-3566. doi:10.1029/2000GL011850

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Published Version: http://dx.doi.org/10.1029/2000GL011850

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Author(s)

J. M. Forbes

Maura E. Hagan-NCAR/UCAR

Title

Diurnal Kelvin wave in the atmosphere of Mars: Towards an understanding of 'stationary' density structures observed by the MGS accelerometer

Publication Title

Geophysical Research Letters

Date

2000-11-01

Volume

Issue

Pages

3563-3566

Resource Type

article

Peer Review

Refereed

Copyright Information

Publisher's Version of Record

http://dx.doi.org/10.1029/2000GL011850

OpenSky Citable URL

http://n2t.net/ark:/85065/d7mp53pq

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Diurnal Kelvin wave in the atmosphere of Mars: Towards an understanding of 'stationary' density structures observed by the MGS accelerometer

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