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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

reflected in the many seminal papers, reviews, and books describing these various processes. Examples of those addressing atmospheric GW topics of most relevance to DEEPWAVE science include the following: GW linear dynamics, propagation, conservation properties, and fluxes ( Hines 1960 ; Eliassen and Palm 1961 ; Bretherton 1969a , b ; Booker and Bretherton 1967 ; Gossard and Hooke 1975 ; Smith 1980 ; Nappo 2013 ); GW sources, characteristics, and responses ( Fritts 1984 ; Fritts and Alexander

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Markus Rapp, Bernd Kaifler, Andreas Dörnbrack, Sonja Gisinger, Tyler Mixa, Robert Reichert, Natalie Kaifler, Stefanie Knobloch, Ramona Eckert, Norman Wildmann, Andreas Giez, Lukas Krasauskas, Peter Preusse, Markus Geldenhuys, Martin Riese, Wolfgang Woiwode, Felix Friedl-Vallon, Björn-Martin Sinnhuber, Alejandro de la Torre, Peter Alexander, Jose Luis Hormaechea, Diego Janches, Markus Garhammer, Jorge L. Chau, J. Federico Conte, Peter Hoor, and Andreas Engel

band of almost zonally symmetric GW activity and related momentum fluxes will be referred to as the “gravity wave belt.” F ig . 1. Illustration of the GW belt based on ERA5 temperature perturbations for (left) August and (right) September 2019 at a pressure levels of 10 hPa. Shown is | T′ | = ⁡ ( T 639 − T 106 ) 2 – (K; see “Models” section for details). The red oval marks the target area where airborne measurements were conducted during SOUTHTRAC-GW. While observational evidence for the GW belt

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