2020
DOI: 10.5194/wcd-2020-21
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On the intermittency of orographic gravity wave hotspots and its importance for middle atmosphere dynamics

Abstract: Abstract. When orographic gravity waves (OGWs) break, they dissipate their momentum and energy and thereby influence the thermal and dynamical structure of the atmosphere. This OGW forcing mainly takes place in the middle atmosphere. It is zonally asymmetric and strongly intermittent. So-called OGW hotspot regions have been shown to exert a large impact on the total wave forcing, in particular in the lower stratosphere (LS). Motivated by this we investigate the asymmetrical distribution of the three-dimensiona… Show more

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Cited by 6 publications
(18 citation statements)
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“…Code and data availability. All processed data files for this study are provided via Mendeley Data (Kuchar, 2020b), and all codes to reproduce our figures are provided via GitHub (Kuchar, 2020a). The authors would like to thank all colleagues involved in the CMAM-sd model simulation (obtained from http://climate-modelling.canada.ca/climatemodeldata/cmam/ output/CMAM/CMAM30-SD/index.shtml, last access: 25 September 2020) (Canadian Centre for Climate Modelling and Analysis, 2020); reanalyses: MERRA-2 (obtained from http://disc.…”
Section: Discussionmentioning
confidence: 99%
“…Code and data availability. All processed data files for this study are provided via Mendeley Data (Kuchar, 2020b), and all codes to reproduce our figures are provided via GitHub (Kuchar, 2020a). The authors would like to thank all colleagues involved in the CMAM-sd model simulation (obtained from http://climate-modelling.canada.ca/climatemodeldata/cmam/ output/CMAM/CMAM30-SD/index.shtml, last access: 25 September 2020) (Canadian Centre for Climate Modelling and Analysis, 2020); reanalyses: MERRA-2 (obtained from http://disc.…”
Section: Discussionmentioning
confidence: 99%
“…Due to the inhomogeneous data distribution, while these spatial clusters represent both large and small scales well, they contain highly uneven numbers of measurements, with a spread of 3 orders of magnitude in population (compared to 5 orders of magnitude using a regular 3° grid). While suitable for mapping, this may introduce spurious intercluster variations in the statistics we compute, namely, the median and Gini's coefficient of concentration G (used previously for GW studies in, e.g., Hindley et al, 2019; Kuchar et al, 2020; Plougonven et al, 2012; Wright et al, 2013). Means were also calculated for all clusters and showed spatially consistent results but with spike values in some clusters due to outliers.…”
Section: Methodsmentioning
confidence: 99%
“…This corresponds to the peak magnitude of the drag during the respective strong OGWD event. As shown in Figure 8 of Kuchar et al (2020), the peak is already preceeded by a few days of significant OGWD anomalies in the region of the hotspot. Therefore, at lag = 0 we can see a response that has already been evolving over a few days prior to lag = 0 under an increasing OGWD forcing overlapping with an imprint of the "hotspot preconditioning."…”
Section: Resultsmentioning
confidence: 92%
“…The selected hotspots are the Rocky Mountains (RM, 235-257.5°E and 27.5-52°N; note that this hotspot was referred to as Western America in Kuchar et al, 2020), the Himalayas (HI, 70-102.5°E and 20-40°N) and Eastern Asia (EA,. These are computed using the peak-detection algorithm described in Kuchar et al (2020). This algorithm identifies peaks (local maxima of negative drag) of OGWD that exceed immediate neighbors separated by more than 20 days with amplitudes beyond a normalized threshold.…”
Section: Methodsmentioning
confidence: 99%
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