A sonic boom propagation model including mean flow atmospheric effects

Author(s):  
Joe Salamone ◽  
Victor W. Sparrow
1963 ◽  
Vol 2 (4) ◽  
pp. 11-14 ◽  
Author(s):  
Domenic J. Maglieri ◽  
Tony L. Parrott

1969 ◽  
Vol 8 (4) ◽  
pp. 618-626 ◽  
Author(s):  
G. A. Herbert ◽  
W. A. Hass ◽  
J. K. Angell

Author(s):  
Gergely Bölöni ◽  
Young-Ha Kim ◽  
Sebastian Borchert ◽  
Ulrich Achatz

AbstractCurrent gravity-wave (GW) parameterization (GWP) schemes are using the steady-state assumption, where an instantaneous balance between GWs and mean flow is postulated, thereby neglecting transient, non-dissipative direct interactions between the GW field and the resolved flow. These schemes rely exclusively on wave dissipation, by GW breaking or near critical layers, as a mechanism leading to forcing of the mean flow. In a transient GWP, without steady-state assumption, non-dissipative direct wave-mean-flow interactions are enabled as an additional mechanism. Idealized studies have shown that this is potentially important, so that the transient GWP Multi-Scale Gravity-Wave Model (MS-GWaM) has been implemented into a state-of-the-art weather and climate model. In this implementation, MS-GWaM leads to a zonal-mean circulation well in agreement with observations, and increases GW momentum-flux intermittency as compared to steady-state GWPs, bringing it into better agreement with super-pressure balloon observations. Transient effects taken into account by MS-GWaM are shown to make a difference even on monthly time-scales: in comparison with steady-state GWPs momentum fluxes in the lower stratosphere are increased and the amount of the missing drag at Southern Hemispheric high latitudes is decreased to a modest but non-negligible extent. An analysis of the contribution of different wavelengths to the GW signal in MS-GWaM suggests that small scale GWs play an important role down to horizontal and vertical wavelengths of 50km (or even smaller) and 200m respectively.


1962 ◽  
Vol 34 (5) ◽  
pp. 720-720
Author(s):  
Domenic J. Maglieri ◽  
Tony L. Parrott

Author(s):  
Sergey Chernyshev ◽  
Andrey Kiselev ◽  
Peter Vorotnikov

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