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dc.date.accessioned 2022-06-24T14:30:24Z
dc.date.available 2022-06-24T14:30:24Z
dc.date.issued 2021
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/138301
dc.description.abstract The southern part of South America and the Antarctic peninsula are known as the world’s strongest hotspot region of stratospheric gravity wave (GW) activity. Large tropospheric winds are deflected by the Andes and the Antarctic Peninsula and excite GWs that might propagate into the upper mesosphere. Satellite observations show large stratospheric GW activity above the mountains, the Drake Passage, and in a belt centered along 60°S. This scientifically highly interesting region for studying GW dynamics was the focus of the Southern Hemisphere Transport, Dynamics, and Chemistry–Gravity Waves (SOUTHTRAC-GW) mission. The German High Altitude and Long Range Research Aircraft (HALO) was deployed to Rio Grande at the southern tip of Argentina in September 2019. Seven dedicated research flights with a typical length of 7,000 km were conducted to collect GW observations with the novel Airborne Lidar for Middle Atmosphere research (ALIMA) instrument and the Gimballed Limb Observer for Radiance Imaging of the Atmosphere (GLORIA) limb sounder. While ALIMA measures temperatures in the altitude range from 20 to 90 km, GLORIA observations allow characterization of temperatures and trace gas mixing ratios from 5 to 15 km. Wave perturbations are derived by subtracting suitable mean profiles. This paper summarizes the motivations and objectives of the SOUTHTRAC-GW mission. The evolution of the atmospheric conditions is documented including the effect of the extraordinary Southern Hemisphere sudden stratospheric warming (SSW) that occurred in early September 2019. Moreover, outstanding initial results of the GW observation and plans for future work are presented. en
dc.format.extent E871-E893 es
dc.language en es
dc.subject Dynamics es
dc.subject Gravity waves es
dc.subject Mountain waves es
dc.subject Stratospheric circulation es
dc.subject Aircraft observations es
dc.title SOUTHTRAC-GW: An airborne field campaign to explore gravity wave dynamics at the world’s strongest hotspot en
dc.type Articulo es
sedici.identifier.other doi:10.1175/bams-d-20-0034.1 es
sedici.identifier.issn 0003-0007 es
sedici.identifier.issn 1520-0477 es
sedici.identifier.issn 1087-3562 es
sedici.creator.person Rapp, Markus es
sedici.creator.person Kaifler, Bernd es
sedici.creator.person Dörnbrack, Andreas es
sedici.creator.person Gisinger, Sonja es
sedici.creator.person Mixa, Tyler es
sedici.creator.person Reichert, Robert es
sedici.creator.person Kaifler, Natalie es
sedici.creator.person Knobloch, Stefanie es
sedici.creator.person Eckert, Ramona es
sedici.creator.person Wildmann, Norman es
sedici.creator.person Giez, Andreas es
sedici.creator.person Krasauskas, Lukas es
sedici.creator.person Preusse, Peter es
sedici.creator.person Geldenhuys, Markus es
sedici.creator.person Riese, Martin es
sedici.creator.person Woiwode, Wolfgang es
sedici.creator.person Friedl-Vallon, Felix es
sedici.creator.person Sinnhuber, Björn-Martin es
sedici.creator.person Torre, Alejandro de la es
sedici.creator.person Alexander, Peter es
sedici.creator.person Hormaechea, José Luis es
sedici.creator.person Janches, Diego es
sedici.creator.person Garhammer, Markus es
sedici.creator.person Chau, Jorge L. es
sedici.creator.person Conte, J. Federico es
sedici.creator.person Hoor, Peter es
sedici.creator.person Engel, Andreas es
sedici.subject.materias Geofísica es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution 4.0 International (CC BY 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Bulletin of the American Meteorological Society es
sedici.relation.journalVolumeAndIssue vol. 102, no. 4 es


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Creative Commons Attribution 4.0 International (CC BY 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution 4.0 International (CC BY 4.0)