Effects of Internal Gravity Waves on Energy Budgets and the Vertical Transport of Angular Momentum Over Mountainous Terrain

1972 ◽  
Vol 100 (3) ◽  
pp. 177-188 ◽  
Author(s):  
GENE L. WOOLDRIDGE
1967 ◽  
Vol 30 (3) ◽  
pp. 439-448 ◽  
Author(s):  
Walter L. Jones

In a rotating system, the vertical transport of angular momentum by internal gravity waves is independent of height, except at critical levels where the Doppler-shifted wave frequency is equal to plus or minus the Coriolis frequency. If slow rotation is ignored in studying the propagation of internal gravity waves through shear flows, the resulting solutions are in error only at levels where the Doppler-shifted and Coriolis frequencies are comparable.


2019 ◽  
Vol 82 ◽  
pp. 247-251
Author(s):  
C. Pinçon ◽  
K. Belkacem ◽  
M.J. Goupil

We investigate the ability of internal gravity waves that are generated by penetrative convection to redistribute angular momentum in the internal radiative zone of evolved low-mass stars. To do so, we use the semianalytical excitation model recently proposed by Pinçon et al.  2016. We briefly report the preliminary results of the study focusing on the subgiant and red giant branch stars.


2013 ◽  
Vol 772 (1) ◽  
pp. 21 ◽  
Author(s):  
T. M. Rogers ◽  
D. N. C. Lin ◽  
J. N. McElwaine ◽  
H. H. B. Lau

2007 ◽  
Vol 474 (1) ◽  
pp. 155-163 ◽  
Author(s):  
F. P. Pantillon ◽  
S. Talon ◽  
C. Charbonnel

2014 ◽  
Vol 796 (1) ◽  
pp. 17 ◽  
Author(s):  
Jim Fuller ◽  
Daniel Lecoanet ◽  
Matteo Cantiello ◽  
Ben Brown

2001 ◽  
Vol 7 (2s) ◽  
pp. 26-33 ◽  
Author(s):  
O.E. Gotynyan ◽  
◽  
V.N. Ivchenko ◽  
Yu.G. Rapoport ◽  
◽  
...  

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