Brentha Thurairajah , Chihoko Y. Cullens , Scott L. England
{"title":"平流层重力波对Madden-Julian振荡的全球响应","authors":"Brentha Thurairajah , Chihoko Y. Cullens , Scott L. England","doi":"10.1016/j.jastp.2025.106584","DOIUrl":null,"url":null,"abstract":"<div><div>The Madden-Julian Oscillation (MJO) is a dominant mode of intraseasonal variability in the tropical troposphere. While the MJO is a slow-moving oscillation that does not propagate to high altitude, it's impacts on the broader spectrum of waves can be seen throughout the middle atmosphere. The influence of this ∼30–90 day oscillation on stratospheric gravity waves (GWs) is not just confined to the tropics but extends to high-latitudes. In this study, we use long-term (1979–2018) reanalysis data to investigate the global stratospheric GW response to MJO during the boreal and austral winter months of December, January, February (DJF) and June, July, August (JJA), respectively. In DJF, the MJO GW relative anomalies are in general significant in both hemispheres during all eight MJO phases. In JJA, the GW relative anomalies are stronger in the winter hemisphere compared to the summer hemisphere. In the low- and mid-latitudes, the GW response in the troposphere depends on the strength of the convection, while the stratospheric response is related to the zonal wind response and filtering of upward propagating GWs. The strength and spatial pattern of GW anomalies in the high-latitude winter hemisphere in MJO Phases 4 and 7 may be connected to the dissipation of MJO related poleward propagating planetary waves.</div></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":"274 ","pages":"Article 106584"},"PeriodicalIF":1.9000,"publicationDate":"2025-06-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Global response of stratospheric gravity waves to Madden-Julian Oscillation\",\"authors\":\"Brentha Thurairajah , Chihoko Y. Cullens , Scott L. England\",\"doi\":\"10.1016/j.jastp.2025.106584\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>The Madden-Julian Oscillation (MJO) is a dominant mode of intraseasonal variability in the tropical troposphere. While the MJO is a slow-moving oscillation that does not propagate to high altitude, it's impacts on the broader spectrum of waves can be seen throughout the middle atmosphere. The influence of this ∼30–90 day oscillation on stratospheric gravity waves (GWs) is not just confined to the tropics but extends to high-latitudes. In this study, we use long-term (1979–2018) reanalysis data to investigate the global stratospheric GW response to MJO during the boreal and austral winter months of December, January, February (DJF) and June, July, August (JJA), respectively. In DJF, the MJO GW relative anomalies are in general significant in both hemispheres during all eight MJO phases. In JJA, the GW relative anomalies are stronger in the winter hemisphere compared to the summer hemisphere. In the low- and mid-latitudes, the GW response in the troposphere depends on the strength of the convection, while the stratospheric response is related to the zonal wind response and filtering of upward propagating GWs. The strength and spatial pattern of GW anomalies in the high-latitude winter hemisphere in MJO Phases 4 and 7 may be connected to the dissipation of MJO related poleward propagating planetary waves.</div></div>\",\"PeriodicalId\":15096,\"journal\":{\"name\":\"Journal of Atmospheric and Solar-Terrestrial Physics\",\"volume\":\"274 \",\"pages\":\"Article 106584\"},\"PeriodicalIF\":1.9000,\"publicationDate\":\"2025-06-23\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Atmospheric and Solar-Terrestrial Physics\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S1364682625001683\",\"RegionNum\":4,\"RegionCategory\":\"地球科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"GEOCHEMISTRY & GEOPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Atmospheric and Solar-Terrestrial Physics","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S1364682625001683","RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
Global response of stratospheric gravity waves to Madden-Julian Oscillation
The Madden-Julian Oscillation (MJO) is a dominant mode of intraseasonal variability in the tropical troposphere. While the MJO is a slow-moving oscillation that does not propagate to high altitude, it's impacts on the broader spectrum of waves can be seen throughout the middle atmosphere. The influence of this ∼30–90 day oscillation on stratospheric gravity waves (GWs) is not just confined to the tropics but extends to high-latitudes. In this study, we use long-term (1979–2018) reanalysis data to investigate the global stratospheric GW response to MJO during the boreal and austral winter months of December, January, February (DJF) and June, July, August (JJA), respectively. In DJF, the MJO GW relative anomalies are in general significant in both hemispheres during all eight MJO phases. In JJA, the GW relative anomalies are stronger in the winter hemisphere compared to the summer hemisphere. In the low- and mid-latitudes, the GW response in the troposphere depends on the strength of the convection, while the stratospheric response is related to the zonal wind response and filtering of upward propagating GWs. The strength and spatial pattern of GW anomalies in the high-latitude winter hemisphere in MJO Phases 4 and 7 may be connected to the dissipation of MJO related poleward propagating planetary waves.
期刊介绍:
The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them.
The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions.
Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.