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  • 1
    Publication Date: 2023-11-28
    Description: Horizontal gravity wave (GW) refraction was observed around the Andes and Drake Passage during the SouthTRAC campaign. GWs interact with the background wind through refraction and dissipation. This interaction helps to drive midatmospheric circulations and slows down the polar vortex by taking GW momentum flux (GWMF) from one location to another. The SouthTRAC campaign was composed to gain improved understanding of the propagation and dissipation of GWs. This study uses observational data from this campaign collected by the German High Altitude Long Range research aircraft on 12 September 2019. During the campaign a minor sudden stratospheric warming in the southern hemisphere occurred, which heavily influenced GW propagation and refraction and thus also the location and amount of GWMF deposition. Observations include measurements from below the aircraft by Gimballed Limb Observer for Radiance Imaging of the Atmosphere and above the aircraft by Airborne Lidar for the Middle Atmosphere. Refraction is identified in two different GW packets as low as ≈4 km and as high as 58 km. One GW packet of orographic origin and one of nonorographic origin is used to investigate refraction. Observations are supplemented by the Gravity‐wave Regional Or Global Ray Tracer, a simplified mountain wave model, ERA5 data and high‐resolution (3 km) WRF data. Contrary to some previous studies we find that refraction makes a noteworthy contribution in the amount and the location of GWMF deposition. This case study highlights the importance of refraction and provides compelling arguments that models should account for this.
    Description: Plain Language Summary: Gravity waves (GWs) are very important for models to reproduce a midatmospheric circulations. But the fact is that models oversimplify the GW physics which results in GWs being underrepresented in models. GW refraction is one of the processes not captured by the physics in model parameterization schemes. This article uses high‐resolution observations from the SouthTRAC campaign to show how GWs refract and highlight the importance there‐of. This case study shows a 25% increase in the GWMF during propagation. The increase in momentum flux is linked to refraction which results in a shortening in the GW horizontal wavelength. This article shows that refraction is important for the amount as well as the location of GWMF deposition. This case study highlights the importance of refraction and provides compelling arguments that models should account for this.
    Description: Key Points: A case study reveals that refraction results in a 25% increase in gravity wave momentum flux (GWMF). Including refraction dynamics affects the location of GWMF deposition. Refraction is prominent in strong wind gradients (i.e., displaced vortex conditions).
    Description: ANPCYT PICT
    Description: DFG
    Description: Bundesministerium für Bildung und Forschung http://dx.doi.org/10.13039/501100002347
    Description: Instituto de Física de Buenos Aires
    Description: SNCAD MinCyT initiative
    Description: HALO‐SPP
    Description: ROMIC WASCLIM
    Description: https://doi.org/10.5281/zenodo.6997443
    Description: https://cds.climate.copernicus.eu/cdsapp%23%21/home
    Keywords: ddc:551.5 ; gravity wave ; mountain wave ; refraction ; Andes ; Drake Passage ; gravity wave momentum flux
    Language: English
    Type: doc-type:article
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  • 2
    Publication Date: 2023-07-21
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Gravity waves (GW) carry energy and momentum from the troposphere to the middle atmosphere and have a strong influence on the circulation there. Global atmospheric models cannot fully resolve GWs, and therefore rely on highly simplified GW parametrizations that, among other limitations, account for vertical wave propagation only and neglect refraction. This is a major source of uncertainty in models, and leads to well‐known problems, such as the late break‐up of polar vortex due to the “missing” GW drag around 60°S. To investigate these phenomena, GW observations over Southern Andes were performed during SouthTRAC aircraft campaign. This paper presents measurements from a SouthTRAC flight on 21 September 2019, including 3‐D tomographic temperature data of the infrared limb imager GLORIA (8–15 km altitude) and temperature profiles of the ALIMA lidar (20–80 km altitude). GLORIA observations revealed multiple overlapping waves of different wavelengths. 3‐D wave vectors were determined from the GLORIA data and used to initialize a GW ray‐tracer. The ray‐traced GW parameters were compared with ALIMA observations, showing good agreement between the instruments and direct evidence of oblique (partly meridional) GW propagation. ALIMA data analysis confirmed that most waves at 25–40 km altitudes were indeed orographic GWs, including waves seemingly upstream of the Andes. We directly observed horizontal GW refraction, which has not been achieved before SouthTRAC. Refraction and oblique propagation caused significant meridional transport of horizontal momentum as well as horizontal momentum exchange between waves and the background flow all along the wave paths, not just in wave excitation and breaking regions.〈/p〉
    Description: Plain Language Summary: Gravity waves (GW) are temperature and wind disturbances in the atmosphere that carry energy and momentum from troposphere to the middle atmosphere and have a strong influence on the circulation there. Global atmospheric models currently cannot adequately represent GW propagation: the facts that GWs can change wavefront orientation (refraction) and travel horizontally (and not just vertically) are typically neglected. This leads to important known model inaccuracies, for example, too low temperatures in southern polar regions. SouthTRAC aircraft measurement campaign observed GWs exited by wind flow over the Southern Andes in September–November 2019. Temperature measurements were conducted with the IR spectrometer GLORIA (provided 3‐D data) and the ALIMA lidar instrument. GLORIA data revealed many overlapping waves of different wavelengths, their propagation further up was investigated using ray‐tracing. Most waves seen by GLORIA were ray‐traced to ALIMA observations where their parameters were confirmed, thus validating our ray‐tracing technique and the two instruments against each other. We directly observed wave propagation in both vertical and horizontal directions and change in horizontal wave orientation (the latter was not seen before SouthTRAC). Due to these phenomena, many GWs carried momentum that had different directions and was deposited in a different location than most models typically predict.〈/p〉
    Description: Key Points: High‐resolution multi‐instrument measurements of orographic gravity waves (GWs) over the Andes were carried out. Oblique GW propagation and strong horizontal refraction were observed and analyzed using ray‐tracing. Significant redistribution of horizontal momentum due to horizontal refraction was observed all along the path of wave propagation.
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: German Ministry for Education and Research
    Description: Bundesministerium für Bildung und Forschung http://dx.doi.org/10.13039/501100002347
    Description: https://www.ecmwf.int/en/forecasts/datasets
    Description: https://doi.org/10.5281/zenodo.7155729
    Keywords: ddc:551.5 ; gravity waves ; refraction ; remote sensing ; lidar ; ray‐tracing
    Language: English
    Type: doc-type:article
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  • 3
    Publication Date: 2024-01-24
    Description: 〈title xmlns:mml="http://www.w3.org/1998/Math/MathML"〉Abstract〈/title〉〈p xmlns:mml="http://www.w3.org/1998/Math/MathML" xml:lang="en"〉Jet streams are important sources of non‐orographic internal gravity waves and clear air turbulence (CAT). We analyze non‐orographic gravity waves and CAT during a merger of the polar front jet stream (PFJ) with the subtropical jet stream (STJ) above the southern Atlantic. Thereby, we use a novel combination of airborne observations covering the meso‐scale and turbulent scale in combination with high‐resolution deterministic short‐term forecasts. Coherent phase lines of temperature perturbations by gravity waves stretching along a highly sheared tropopause fold are simulated by the ECMWF IFS (integrated forecast system) forecasts. During the merging event, the PFJ reverses its direction from approximately antiparallel to parallel with respect to the STJ, going along with strong wind shear and horizontal deformation. Temperature perturbations in limb‐imaging and lidar observations onboard the research aircraft HALO during the SouthTRAC campaign show remarkable agreement with the IFS data. Ten hours earlier, the IFS data show an “X‐shaped” pattern in the temperature perturbations emanating from the sheared tropopause fold. Tendencies of the IFS wind components show that these gravity waves are excited by spontaneous emission adjusting the strongly divergent flow when the PFJ impinges the STJ. In situ observations of temperature and wind components at 100 Hz confirm upward propagation of the probed portion of the gravity waves. They furthermore reveal embedded episodes of light‐to‐moderate CAT, Kelvin Helmholtz waves, and indications for partial wave reflection. Patches of low Richardson numbers in the IFS data coincide with the CAT observations, suggesting that this event was accessible to turbulence forecasting.〈/p〉
    Description: Plain Language Summary: Gravity waves play an in important role in vertical and horizontal energy transport in the atmosphere and are significant factors in wheather forecasting and climate projections. Among other processes, tropospheric jet streams are known to be sources of gravity waves. They furthermore can be accompanied by tropopause folds (i.e., local tropopause depressions, where stratospheric air can reach deeply into the troposphere) and turbulence, which is relevant for aviation safety. Using a novel combination of airborne observations and data by a state‐of‐the‐art forecasting system, we analyze gravity waves and turbulence during a merger of tropospheric jet streams above the southern Atlantic. The observations show a high degree of agreement with the forecast data from the troposphere to the stratosphere. Ten hours earlier, the forcast data show an “X‐shaped” gravity wave structure that emerges from a highly sheared tropopause fold between the merging jet streams. Fast in situ observations at the flight level provide information on the characteristics of the observed waves and show light‐to‐moderate turbulence, small‐scale waves and indications for partial wave reflection. The observed turbulence events are consistently located in regions where the forecast data suggest potential for turbulence.〈/p〉
    Description: Key Points: 〈list list-type="bullet"〉 〈list-item〉 〈p xml:lang="en"〉Non‐orographic internal gravity waves and clear air turbulence are observed in merging jet streams〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉State‐of‐the art high resolution forecast agrees with novel combination of airborne sensors〈/p〉〈/list-item〉 〈list-item〉 〈p xml:lang="en"〉“X‐shaped” gravity wave feature resulting from merging jet streams at a highly sheared tropopause fold〈/p〉〈/list-item〉 〈/list〉 〈/p〉
    Description: Bundesministerium für Bildung und Forschung http://dx.doi.org/10.13039/501100002347
    Description: Deutsche Forschungsgemeinschaft http://dx.doi.org/10.13039/501100001659
    Description: https://doi.org/10.5445/IR/1000151856
    Description: https://www.ecmwf.int/en/forecasts
    Description: https://www.ready.noaa.gov/
    Keywords: ddc:551.5 ; gravity waves ; jet streams ; clear air turbulence ; remote sensing ; in situ observations ; field campaigns
    Language: English
    Type: doc-type:article
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  • 4
    Publication Date: 2023-07-01
    Description: To improve our knowledge of the coupling of atmospheric circulation, composition and regional climate, and to provide the urgently needed observations of long-term changes in the middle atmosphere, the Changing-Atmosphere Infra-Red Tomography Explorer (CAIRT) is one of four mission concepts down-selected by the European Space Agency (ESA) for competitive pre-feasibility studies, vying for implementation as the next Earth Explorer satellite mission. As a Fourier transform infrared limb imager, CAIRT will observe simultaneously from the middle troposphere to the lower thermosphere at high spectral resolution and with unprecedented horizontal and vertical resolution (with a goal of 50×50×1 km globally). With this, CAIRT will provide new and critical information on (a) atmospheric gravity waves, circulation and mixing, (b) coupling with the upper atmosphere, solar variability and space weather and, (c) aerosols and pollutants in the upper troposphere and lower stratosphere. In this presentation we will give an overview of CAIRT’s science goals and the expected mission performance, based on latest results from early mission definition studies.
    Language: English
    Type: info:eu-repo/semantics/conferenceObject
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  • 5
    Publication Date: 2023-08-09
    Description: We investigate the GW dynamics in the 2006 Sudden Stratospheric Warming by means of a high resolution run of the ECMWF-IFS. With initial condition from ERA-5 the ECMWF-IFS GCM was run at TCo2559 spatial resolution (corresponding to a 4.5~km horizontal grid) for 42 hrs in forecasting mode and data for this analysis stored at 24, 30, 36 and 42 hrs. These data were investigated by the small-volume sinusoidal fit method (S3D) resulting in 3D wave vectors, amplitudes and phases of temperature and vertical wind for up to 4 wave components. By comparing phase information from temperature and vertical wind, wave events can be separated for upward and downward propagation. In the days before the break-up of the vortex, gravity wave momentum flux shows a dipole of eastward and westward flux around the vortex edge. We will investigate the generation and corresponding drag of this pattern in detail. In addition we will demonstrate how a novel type of space-borne limb imager, the CAIRT mission proposed for EE11, could gain such information from actual observations. We will highlight the step change such a novel type of observations could make compared to the best available data set, i.e. HIRDLS GW analyses, from this period, which was the golden year of stratospheric GW observations.
    Language: English
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  • 6
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    In:  XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG)
    Publication Date: 2023-06-28
    Description: The uncertainty in gravity wave (GW) parameterizations in conventional general circulation models has so far prevented a conclusive answer on how GWs, their interaction with the quasi-biennial oscillation (QBO), and the QBO itself may change in a warming climate. In this study, we therefore performed short explicit simulations of the QBO for different idealized climate states with the deep convection-permitting model ICON, which does not employ a parameterization of either deep convection or GWs. Thus, the QBO is entirely driven by explicitly resolved waves. Thereby, our simulations allow us to provide a very first direct estimate of how tropical GWs and the QBO may change in a warming climate.We find that a warmer climate results in a more vigorous generation of GWs by deep convection, resulting in a substantial increase of the lower-stratospheric GW momentum flux at phase speeds relevant for the QBO. As a consequence, the QBO downward propagation accelerates in the warmer climate states. Additionally, the dominant phase speed of the GW spectrum tends to increase in the warmer climate states, accompanied by a strengthening of the QBO jets in the upper QBO domain.We conclude that our results have qualitatively constrained potential changes in stratospheric GW momentum flux due to a warming climate and in view of this a warming-induced acceleration of the QBO seems to become increasingly likely. In a next step, we plan to extend some simulations to a longer time period to get a more comprehensive assessment of potential QBO changes in a warming climate.
    Language: English
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  • 7
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    In:  XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG)
    Publication Date: 2023-07-10
    Description: The Polar Environment Atmospheric Research Laboratory (PEARL), established in 2005 at Eureka, Nunavut, Canada on Ellesmere Island (80N 85W), provides observations of the polar atmosphere from the ground to the lower thermosphere. Observations of wave signatures using an all-sky imager and the E-Region Wind Interferometer (ERWIN) with periods from 10’s of minutes to ~14 hours are examined. Horizontal winds are intermittent and the amplitude spectra peak in the 6 – 12 hour period region. This peak is not seen in the vertical wind and airglow brightness spectra. It appears that waves in this period range are not tidal in nature but are inertial gravity waves. A few wave events with periods of ~3 hours have been analysed using a gravity wave ray tracing program (GROGRAT) and found to be related to strong tropospheric storms. Short period gravity waves were also identified in the imager observation and explored using GROTGRAT. Their observed characteristics, suggest they are secondary waves associated with orographic gravity wave dissipation. The variety of characteristics and sources of these waves point to the complex nature of waves propagating into the polar ionosphere.
    Language: English
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  • 8
    Publication Date: 2023-07-11
    Description: The Changing-Atmosphere Infra-Red Tomography Explorer (CAIRT) is one of the four candidates for ESA’s Earth Explorer 11, aimed to study the coupling between atmospheric composition, circulation and climate. By exploiting its imaging capabilities, CAIRT indeed can sound the atmosphere simultaneously from the middle troposphere to the lower thermosphere at 0.2 cm〈sup〉-1〈/sup〉 spectral resolution and with horizontal sampling of 50 km along track, 50 km across track and vertical sampling of 1 km. Flying in loose formation with MetOp-SG mission allows to combine spatially resolved limb observations with horizontally resolved nadir measurements of IASI-NG and Sentinel-5 nadir spectrometers to extend limb observations down to the surface. An accurate knowledge of trace gas composition around the tropopause is particularly important to reduce significant uncertainties in projected future warming: changes in the surface air pollution and in the stratosphere-troposphere exchange may significantly affect it. Moreover quantifying the influence of stratospheric transport on near-surface tropospheric composition is important since it conditions attempts to derive emission fluxes from surface observations for important greenhouse gases. We evaluated advantages coming from the exploitation of the synergy between realistic simulations of CAIRT, IASI-NG and Sentinel 5 observations applying the rigorous approach of the two-dimensional complete data fusion. The synergistic products demonstrate a better quality in sounding both the troposphere and the Upper Troposphere - Lower Stratosphere region. Results will be shown for selected case studies involving ozone, methane and other pollutants.
    Language: English
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  • 9
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    In:  XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG)
    Publication Date: 2023-07-13
    Description: The Swedish satellite MATS was launched in November 2022. MATS derives three-dimensional temperature fields from the mesosphere and lower thermosphere by observing atmospheric airglow emissions and light scattered off noctilucent clouds. As propagating gravity waves introduce fluctuations in pressure, density and temperature, these measurements can be used to study the wave dynamics of this energetic atmospheric region. To correctly capture the gravity wave spectra, wave-induced perturbations have to be isolated from larger scale fluctuations of the background atmosphere. Based on measurements made by MATS during the initial operational months, as well as synthetic tomography data, we investigate how waves affect the MATS measurements, and how their properties can be derived.
    Language: English
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  • 10
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    In:  XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG)
    Publication Date: 2023-09-18
    Description: In order to investigate the driving of the QBO a high-resolution, convection-permitting run of the ICON model with 5km grid spacing was performed. Neither convection nor gravity waves (GWs) were parametrized. Here we analyze the resolved GWs in the model data by applying a small-volume sinusoidal fit method (S3D). By using a cascade of cube sizes, horizontal wavelengths of 150km - 2000km are addressed. This acts as a compromise between spectral resolution and spatial location. Phase speed spectra and gravity wave momentum flux (GWMF) can be reconstructed for individual regions and single snap-shots. Via the comparison of phases from wave fits of temperature and winds, the vertical propagation direction of individual waves can be separated and ray-tracing can be initialized accordingly. Using the results of this analysis we study the effect of the critical level GW filtering by comparing the vertical variation of phase speed spectra by means of blocking diagrams. Despite the generally good agreement, GWs with unexpected phase speeds at given altitudes due to critical level filtering are present. Multiple potential reasons are identified. Ray-tracing studies are carried out to investigate the potential influence of these various processes and quantify deviations from simple propagation and filtering assumptions used in GW parametrizations. The origin of these GWs is investigated and the regional variation of the blocking due to wind filtering is studied in more detail. Further, a ray-tracing is initialized using the results to improve the understanding of the role of horizontal GW propagation when compared to GW parametrization.
    Language: English
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