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  • Planetary waves x
  • DEEPWAVE: The Deep Propagating Gravity Wave Experiment x
  • Multi-Scale Dynamics of Gravity Waves (MS-GWaves) x
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Sonja Gisinger, Andreas Dörnbrack, Vivien Matthias, James D. Doyle, Stephen D. Eckermann, Benedikt Ehard, Lars Hoffmann, Bernd Kaifler, Christopher G. Kruse, and Markus Rapp

information about the various datasets used in this study. In section 3 , we discuss specific tropospheric flow regimes and forcing conditions during DEEPWAVE. Section 4 is devoted to the tropopause layer. The stratospheric and mesospheric wind and thermal conditions providing the ambient atmospheric profiles for deep propagating gravity waves are described in section 5 . There, planetary wave activity and its impact on the location of the PNJ and the polar vortex are discussed. Special attention is

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Benedikt Ehard, Peggy Achtert, Andreas Dörnbrack, Sonja Gisinger, Jörg Gumbel, Mikhail Khaplanov, Markus Rapp, and Johannes Wagner

), which turn out to be periods when mountain waves were excited by the flow across the Scandinavian mountain ridge. These perturbations are correlated with an enhanced tropospheric wind and a jet stream near the tropopause ( Fig. 2b ). Most noticeable are the downward-propagating wind anomalies in the period 3–4 December 2013. The upper-stratospheric and mesospheric winds show a remarkable variability, which probably results from planetary waves disturbing the polar vortex during this period. Fig . 2

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Tanja C. Portele, Andreas Dörnbrack, Johannes S. Wagner, Sonja Gisinger, Benedikt Ehard, Pierre-Dominique Pautet, and Markus Rapp

linear mountain-wave theory ( Smith 1979 ). Moreover, there are numerous numerical studies about transiently forced mountain waves. Lott and Teitelbaum (1993a , b ) investigated the wave dynamics in a 2D linear time-dependent model with transient incident stably stratified flow. Chen et al. (2005 , 2007 ) and Hills and Durran (2012) extended the work of Lott and Teitelbaum (1993a , b ) and studied the impact of the flow of a time-dependent barotropic planetary square wave in a uniformly

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David C. Fritts, Ronald B. Smith, Michael J. Taylor, James D. Doyle, Stephen D. Eckermann, Andreas Dörnbrack, Markus Rapp, Bifford P. Williams, P.-Dominique Pautet, Katrina Bossert, Neal R. Criddle, Carolyn A. Reynolds, P. Alex Reinecke, Michael Uddstrom, Michael J. Revell, Richard Turner, Bernd Kaifler, Johannes S. Wagner, Tyler Mixa, Christopher G. Kruse, Alison D. Nugent, Campbell D. Watson, Sonja Gisinger, Steven M. Smith, Ruth S. Lieberman, Brian Laughman, James J. Moore, William O. Brown, Julie A. Haggerty, Alison Rockwell, Gregory J. Stossmeister, Steven F. Williams, Gonzalo Hernandez, Damian J. Murphy, Andrew R. Klekociuk, Iain M. Reid, and Jun Ma

, temperatures, and turbulence from ∼30 to 100 km and enabled studies of energy dissipation rates due to GW breaking, MW filtering during a stratospheric warming, and anomalous MLT mean structure accompanying strong planetary waves (PWs) in the Southern Hemisphere and other dynamics (e.g., Rapp et al. 2004 ; Wang et al. 2006 ; Goldberg et al. 2006 ). Multiple types of radars have quantified GW amplitudes, scales, spectral character, momentum fluxes, and evidence of various interaction and instability

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