Wave transport in differentially rotating stellar radiation zones

Details Wave transport in differentially rotating stellar radiation zones Wave transport in differentially rotating stellar radiation zones

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coast.157..209m&link_type=abstract

Communications in Asteroseismology, Vol.157, p. 209-215

Computer Science

1

Scientific paper

In this work, the complete interaction between low-frequency internal gravity waves and differential rotation in stably strongly stratified stellar radiation zones is examined. First, the modification of the structure of those waves due to the Coriolis acceleration is obtained. Then, their feed-back on the angular velocity profile through their induced angular momentum transport is derived. Finally, perspectives are discussed.

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