Atmos. Chem. Phys., 18, 15643–15667, 2018 https://doi.org/10.5194/acp-18-15643-2018 © Author(s) 2018. This work is distributed under the Creative Commons Attribution 4.0 License. Mesoscale fine structure of a tropopause fold over mountains Wolfgang Woiwode1, Andreas Dörnbrack2, Martina Bramberger2, Felix Friedl-Vallon1, Florian Haenel1, Michael Höpfner1, Sören Johansson1, Erik Kretschmer1, Isabell Krisch3, Thomas Latzko1, Hermann Oelhaf1, Johannes Orphal1, Peter Preusse3, Björn-Martin Sinnhuber1, and Jörn Ungermann3 1Institute of Meteorology and Climate Research, Karlsruhe Institute of Technology, Karlsruhe, Germany 2Deutsches Zentrum für Luft- und Raumfahrt, Institut für Physik der Atmosphäre, Oberpfaffenhofen, Germany 3Forschungszentrum Jülich, Institute of Energy- and Climate Research, Stratosphere (IEK-7), Jülich, Germany Correspondence: Wolfgang Woiwode ([email protected]) Received: 22 June 2018 – Discussion started: 10 July 2018 Revised: 13 September 2018 – Accepted: 21 September 2018 – Published: 30 October 2018 Abstract. We report airborne remote-sensing observations 1 Introduction of a tropopause fold during two crossings of the polar front jet over northern Italy on 12 January 2016. The GLORIA (Gimballed Limb Observer for Radiance Imaging of the At- Tropopause folds are preferred regions of bidirectional mosphere) observations allowed for a simultaneous map- stratosphere–troposphere exchange (STE) of mass and trace ping of temperature, water vapour, and ozone. They revealed gases in the middle latitudes (e.g. Holton et al., 1995; Get- deep, dry, and ozone-rich intrusions into the troposphere. telman et al., 2011, and references therein). Their generation The mesoscale fine structures of dry filaments at the cyclonic is related to cyclogenetically active regions (e.g. Keyser and shear side north of the jet and tongues of moist air entraining Shapiro, 1986, and references therein), which develop nar- tropospheric air into the stratosphere along the anticyclonic row transition zones where all flow variables become very shear side south of the jet were clearly resolved by GLO- concentrated. The associated formation of upper-level fronts RIA observations. Vertically propagating mountain waves and surface fronts is mainly driven by the nonlinear self- with recorded temperature residuals exceeding ± 3 K were advection of evolving Rossby waves. Tropopause folds form detected above the Apennines. Their presence enhanced gra- preferentially along strong jet streams separating polar or dients of all variables locally in the vicinity of the tropopause. Arctic air masses from those of subtropical origin. The po- lar front jet (PFJ) is found at middle latitudes and is of- The combination of H2O−O3 correlations with potential temperature reveals an active mixing region and shows clear ten classified as an eddy-driven jet stream (Held, 1975; Lee evidence of troposphere-to-stratosphere and stratosphere-to- and Kim, 2003). Upper-level jet and front systems are prone troposphere exchange. High-resolution short-term determin- to the generation of clear-air turbulence, which is an im- istic forecasts of ECMWF’s integrated forecast system (IFS) portant exchange mechanism for atmospheric constituents applying GLORIA’s observational filter reproduce location, across the tropopause (e.g. Shapiro, 1978, 1980; Koch et al., shape, and depth of the tropopause fold very well. The fine 2005; Kühnlein, 2006; Sharman et al., 2012). Extratropical structure of the mixing region, however, cannot be repro- jet streams are waveguides for planetary Rossby waves (e.g. duced even with the 9 km horizontal resolution of the IFS, Dritschel and McIntyre, 2008; Martius et al., 2010). More- used here. This case study demonstrates convincingly the over, they provide a favourable medium for the vertical prop- capabilities of linear limb-imaging observations to resolve agation of internal gravity waves excited in the troposphere mesoscale fine structures in the upper troposphere and lower (e.g. Preusse et al., 2006; Ern et al., 2018). stratosphere, validates the high quality of the IFS data, and Observations of tropopause folds go back to the middle suggests that mountain wave perturbations have the potential of the last century when their spatial structure was por- to modulate exchange processes in the vicinity of tropopause trayed by observations from radio soundings distributed over folds. large horizontal distances (Reed, 1955; Reed and Danielsen, 1958; historical review by Keyser and Shapiro, 1986). Later, Published by Copernicus Publications on behalf of the European Geosciences Union. 15644 W. Woiwode et al.: Mesoscale fine structure of a tropopause fold and due to the urgent need to explain the exceptional max- technique enables much higher sampling rates as all vertical imum springtime radioactive fallout over North America, viewing angles associated with a set of atmospheric parame- the first coordinated aircraft observations were undertaken ter profiles are measured at the same time. (Danielsen, 1964, 1968; Danielsen and Mohnen, 1977). Be- The horizontal viewing characteristic of GLORIA plays sides atmospheric variables such as wind and temperature, an important role. In cases of horizontally elongated features they sampled trace gases, radio nuclei, and aerosols along (i.e. several hundreds of kilometres) such as tropopause folds stacked flight legs through jet streams. Their composites along the jet stream, the along-track sampling of GLORIA combining potential temperature, potential vorticity, and var- can resolve vertical cross sections in high detail by choos- ious constituents enhanced our knowledge about the spatial ing flight tracks perpendicular to the jet axis. Thereby, GLO- structure of tropopause folds and the contributions of advec- RIA’s low horizontal direction resolution along the line of tion, mixing, and radiation to STE. Melvin Shapiro brought sight is directed along the elongated atmospheric feature, those early conceptual plots by Reed and Danielsen to per- while the dense along-track sampling is exploited to resolve fection and designed 2-D cross sections of potential tem- structures across the jet axis. perature, wind, ozone, and condensation nuclei from flight In the past, temperature in tropopause folds along the ver- level and dropsonde measurements (Shapiro, 1980). Basi- tical direction was observed at flight level and by dropsondes cally, these conceptual visualizations provided the base for underneath. Simultaneous in situ measurements of both trace modified and refined schematics in recent publications (e.g. gases and temperature have not been applied up to now to see Fig. 1 in Gettelman et al., 2011). Later, airborne li- characterize the mesoscale fine structure of tropopause folds. dar observations using the differential absorption lidar tech- CRISTA-NF observations in July 2006 (Weigel et al., 2012) nique provided valuable insights into the spatial structure of provided a first coarse perspective of a tropopause fold us- tropopause folds (e.g. Browell, 1987; Ehret, 1999; Flentje, ing this combination of parameters. Here, we present GLO- 2005). Airborne observations by one lidar mostly give mix- RIA airborne observations of temperature, water vapour, ing ratios of one atmospheric constituent (e.g. water vapour and ozone taken simultaneously during two passages of or ozone) and aerosol backscatter. Simultaneous airborne li- a tropopause fold located over northern Italy on 12 Jan- dar observations of ozone and water vapour were only pos- uary 2016 in unprecedented quality. GLORIA was deployed sible on large platforms such as NASA’s DC8 (Kooi et al., on board the HALO during the merged campaigns POL- 2008), and, most recently, on the German research aircraft STRACC (POLar STRAtosphere in a Changing Climate), HALO (High Altitude and Long Range Research Aircraft) GW-LCYCLE II (Investigation of the life cycle of gravity during a mission over the North Atlantic (Andreas Schäfler, waves), and SALSA (Seasonality of Air mass transport and personal communication, 2018). origin in the Lowermost Stratosphere using the HALO Air- Limb observations of various trace gases from a high- craft), in the following abbreviated as PGS. Goals of the PGS flying research aircraft were analysed by Weigel et al. (2012) campaign were atmospheric and chemical observations re- and Ungermann et al. (2013) to investigate their filamentary lated to the Arctic stratospheric polar vortex, gravity waves, structure in the summer-time extratropical transition layer and the seasonality of air mass exchange in the UTLS. near the subtropical jet stream (STJ). The Cryogenic In- GLORIA observations along two extended legs of the re- frared Spectrometers and Telescope for the Atmosphere – search flight over northern Italy reveal the existence of a New Frontiers (CRISTA-NF) resolved filaments of a spa- deep stratospheric intrusion wrapping around the PFJ. At the tial scale of less than 800 m vertically. The diagnostics ap- same time, mountain waves excited by the strong low-level plied (tracer–tracer correlations of PAN and O3) provided flow over the Apennines propagated vertically from the tro- the first multi-species 2-D portrait of the inhomogeneous posphere into the stratosphere. Both the south- and north- distributions within a tropopause fold extending from about bound flight legs were oriented nearly perpendicularly to the 14 down to 8 km altitude. Moreover, infrared limb observa- axis of the PFJ. Therefore, GLORIA probed the tropopause tions are capable of resolving gravity
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