Sharon L. Vadas, David R. Themens, Joseph D. Huba, Erich Becker, Katrina Bossert, Larisa Goncharenko, Sophie J. Maguire, Cosme A. O. B. Figueiredo, Shuang Xu, V. Lynn Harvey, Nathaniel A. Frissell, Michael J. Molzen, Thomas J. Pisano, Grzegorz Nykiel
{"title":"2016年1月11-15日极地涡旋急流的高阶重力波和行电离层扰动:HIAMCM-SAMI3模拟及与热层和电离层观测的比较","authors":"Sharon L. Vadas, David R. Themens, Joseph D. Huba, Erich Becker, Katrina Bossert, Larisa Goncharenko, Sophie J. Maguire, Cosme A. O. B. Figueiredo, Shuang Xu, V. Lynn Harvey, Nathaniel A. Frissell, Michael J. Molzen, Thomas J. Pisano, Grzegorz Nykiel","doi":"10.1029/2024JA033040","DOIUrl":null,"url":null,"abstract":"<p>In Vadas et al. (2024, https://doi.org/10.1029/2024ja032521), we modeled the atmospheric gravity waves (GWs) during 11–14 January 2016 using the HIAMCM, and found that the polar vortex jet generates medium to large-scale, higher-order GWs in the thermosphere. In this paper, we model the traveling ionospheric disturbances (TIDs) generated by these GWs using the HIAMCM-SAMI3 and compare with ionospheric observations from ground-based Global Navigation Satellite System (GNSS) receivers, Incoherent Scatter Radars (ISR) and the Super Dual Auroral Radar Network (SuperDARN). We find that medium to large-scale TIDs are generated worldwide by the higher-order GWs from this event. Many of the TIDs over Europe and Asia have concentric ring/arc-like structure, and most of those over North/South America have planar wave structure and occur during the daytime. Those over North/South America propagate southward and are generated by higher-order GWs from Europe/Asia which propagate over the Arctic. These latter TIDs can be misidentified as arising from geomagnetic forcing. We find that the higher-order GWs that propagate to Africa and Brazil from Europe may aid in the formation of equatorial plasma bubbles (EPBs) there. We find that the simulated GWs, TIDs and EPBs agree with EISCAT, PFISR, GNSS, and SuperDARN measurements. We find that the higher-order GWs are concentrated at <span></span><math>\n <semantics>\n <mrow>\n <mn>60</mn>\n <mo>−</mo>\n <mn>90</mn>\n <mo>°</mo>\n </mrow>\n <annotation> $60-90{}^{\\circ}$</annotation>\n </semantics></math>N at <span></span><math>\n <semantics>\n <mrow>\n <mi>z</mi>\n <mspace></mspace>\n <mo>≥</mo>\n </mrow>\n <annotation> $z\\ \\ge $</annotation>\n </semantics></math> 200 km, in agreement with GOCE and CHAMP data. Thus the polar vortex jet is important for generating TIDs in the northern winter ionosphere via multi-step vertical coupling through GWs.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":"130 1","pages":""},"PeriodicalIF":2.9000,"publicationDate":"2024-12-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Higher-Order Gravity Waves and Traveling Ionospheric Disturbances From the Polar Vortex Jet on 11–15 January 2016: Modeling With HIAMCM-SAMI3 and Comparison With Observations in the Thermosphere and Ionosphere\",\"authors\":\"Sharon L. Vadas, David R. Themens, Joseph D. Huba, Erich Becker, Katrina Bossert, Larisa Goncharenko, Sophie J. Maguire, Cosme A. O. B. Figueiredo, Shuang Xu, V. Lynn Harvey, Nathaniel A. Frissell, Michael J. Molzen, Thomas J. Pisano, Grzegorz Nykiel\",\"doi\":\"10.1029/2024JA033040\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>In Vadas et al. (2024, https://doi.org/10.1029/2024ja032521), we modeled the atmospheric gravity waves (GWs) during 11–14 January 2016 using the HIAMCM, and found that the polar vortex jet generates medium to large-scale, higher-order GWs in the thermosphere. In this paper, we model the traveling ionospheric disturbances (TIDs) generated by these GWs using the HIAMCM-SAMI3 and compare with ionospheric observations from ground-based Global Navigation Satellite System (GNSS) receivers, Incoherent Scatter Radars (ISR) and the Super Dual Auroral Radar Network (SuperDARN). We find that medium to large-scale TIDs are generated worldwide by the higher-order GWs from this event. Many of the TIDs over Europe and Asia have concentric ring/arc-like structure, and most of those over North/South America have planar wave structure and occur during the daytime. Those over North/South America propagate southward and are generated by higher-order GWs from Europe/Asia which propagate over the Arctic. These latter TIDs can be misidentified as arising from geomagnetic forcing. We find that the higher-order GWs that propagate to Africa and Brazil from Europe may aid in the formation of equatorial plasma bubbles (EPBs) there. We find that the simulated GWs, TIDs and EPBs agree with EISCAT, PFISR, GNSS, and SuperDARN measurements. We find that the higher-order GWs are concentrated at <span></span><math>\\n <semantics>\\n <mrow>\\n <mn>60</mn>\\n <mo>−</mo>\\n <mn>90</mn>\\n <mo>°</mo>\\n </mrow>\\n <annotation> $60-90{}^{\\\\circ}$</annotation>\\n </semantics></math>N at <span></span><math>\\n <semantics>\\n <mrow>\\n <mi>z</mi>\\n <mspace></mspace>\\n <mo>≥</mo>\\n </mrow>\\n <annotation> $z\\\\ \\\\ge $</annotation>\\n </semantics></math> 200 km, in agreement with GOCE and CHAMP data. 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引用次数: 0
摘要
Vadas et al. (2024, https://doi.org/10.1029/2024ja032521)利用HIAMCM对2016年1月11-14日的大气重力波(GWs)进行了模拟,发现极涡射流在热层产生中到大尺度、高阶的重力波。本文利用HIAMCM-SAMI3模拟了这些GWs产生的电离层扰动(TIDs),并与地面全球导航卫星系统(GNSS)接收机、非相干散射雷达(ISR)和超级双极光雷达网(superdual oral Radar Network)的电离层观测结果进行了比较。我们发现,这次事件的高阶GWs在全球范围内产生了中到大规模的tid。欧洲和亚洲的许多tid具有同心圆环形/弧形结构,而北美/南美的大多数tid具有平面波结构,并且发生在白天。北美/南美上空的那些向南传播,是由欧洲/亚洲在北极上空传播的高阶GWs产生的。这些后一种tid可能被误认为是由地磁强迫引起的。我们发现,从欧洲传播到非洲和巴西的高阶GWs可能有助于赤道等离子体气泡(EPBs)的形成。我们发现模拟的GWs、TIDs和EPBs与EISCAT、PFISR、GNSS和SuperDARN测量值一致。我们发现,在z≥$z\ \ge $ 200 km处,高阶GWs集中在60 ~ 90°$60 ~ 90{}^{\circ}$ N处,与GOCE和CHAMP数据一致。因此,极地涡旋急流通过GWs的多阶垂直耦合在北方冬季电离层产生tid是重要的。
Higher-Order Gravity Waves and Traveling Ionospheric Disturbances From the Polar Vortex Jet on 11–15 January 2016: Modeling With HIAMCM-SAMI3 and Comparison With Observations in the Thermosphere and Ionosphere
In Vadas et al. (2024, https://doi.org/10.1029/2024ja032521), we modeled the atmospheric gravity waves (GWs) during 11–14 January 2016 using the HIAMCM, and found that the polar vortex jet generates medium to large-scale, higher-order GWs in the thermosphere. In this paper, we model the traveling ionospheric disturbances (TIDs) generated by these GWs using the HIAMCM-SAMI3 and compare with ionospheric observations from ground-based Global Navigation Satellite System (GNSS) receivers, Incoherent Scatter Radars (ISR) and the Super Dual Auroral Radar Network (SuperDARN). We find that medium to large-scale TIDs are generated worldwide by the higher-order GWs from this event. Many of the TIDs over Europe and Asia have concentric ring/arc-like structure, and most of those over North/South America have planar wave structure and occur during the daytime. Those over North/South America propagate southward and are generated by higher-order GWs from Europe/Asia which propagate over the Arctic. These latter TIDs can be misidentified as arising from geomagnetic forcing. We find that the higher-order GWs that propagate to Africa and Brazil from Europe may aid in the formation of equatorial plasma bubbles (EPBs) there. We find that the simulated GWs, TIDs and EPBs agree with EISCAT, PFISR, GNSS, and SuperDARN measurements. We find that the higher-order GWs are concentrated at N at 200 km, in agreement with GOCE and CHAMP data. Thus the polar vortex jet is important for generating TIDs in the northern winter ionosphere via multi-step vertical coupling through GWs.