T. Bozóki, J. Mlynarczyk, E. Prácser, A. Kulak, G. Sátori, M. Füllekrug, E. Williams
In lightning research, there is a growing interest in measuring the extremely low frequency (ELF, 3 Hz–3 kHz) electromagnetic (EM) radiation of lightning, as this frequency band can be used to infer various characteristics of lightning discharges that are currently not available from state-of-the-art lightning detection networks. One of these characteristics is the presence of a continuing current (CC), which can last for hundreds of milliseconds and therefore poses an increased risk of physical lightning damage. In this paper, we investigate the modeling capability of the global EM resonance field excited by lightning with a CC using a modified version of a well-known analytical model describing Schumann resonances (SRs) and a full FDTD model. Since analytical models are much faster and require significantly less memory than full numerical models, they are widely used to interpret ELF data. On the other hand, the flexibility of a full numerical model allows the simulation of model configurations that cannot be described by analytical models. To use the two models confidently, it is important to check their consistency for similar configurations. Here, we demonstrate that, for a uniform Earth-ionosphere cavity, the theoretical ELF spectra provided by the analytical and full numerical models show good agreement ∼7(±5) % for both the impulse-like (describing SRs) and exponentially decaying (describing the presence of a CC) current sources. Our results confirm that the analytical model is well suited to interpret ELF measurements for the purpose of studying global lightning activity or individual lightning discharges.
{"title":"Modeling the Global Electromagnetic Resonance Field Produced by Lightning Discharges With a Continuing Current","authors":"T. Bozóki, J. Mlynarczyk, E. Prácser, A. Kulak, G. Sátori, M. Füllekrug, E. Williams","doi":"10.1029/2025JD043989","DOIUrl":"https://doi.org/10.1029/2025JD043989","url":null,"abstract":"<p>In lightning research, there is a growing interest in measuring the extremely low frequency (ELF, 3 Hz–3 kHz) electromagnetic (EM) radiation of lightning, as this frequency band can be used to infer various characteristics of lightning discharges that are currently not available from state-of-the-art lightning detection networks. One of these characteristics is the presence of a continuing current (CC), which can last for hundreds of milliseconds and therefore poses an increased risk of physical lightning damage. In this paper, we investigate the modeling capability of the global EM resonance field excited by lightning with a CC using a modified version of a well-known analytical model describing Schumann resonances (SRs) and a full FDTD model. Since analytical models are much faster and require significantly less memory than full numerical models, they are widely used to interpret ELF data. On the other hand, the flexibility of a full numerical model allows the simulation of model configurations that cannot be described by analytical models. To use the two models confidently, it is important to check their consistency for similar configurations. Here, we demonstrate that, for a uniform Earth-ionosphere cavity, the theoretical ELF spectra provided by the analytical and full numerical models show good agreement ∼7(±5) % for both the impulse-like (describing SRs) and exponentially decaying (describing the presence of a CC) current sources. Our results confirm that the analytical model is well suited to interpret ELF measurements for the purpose of studying global lightning activity or individual lightning discharges.</p>","PeriodicalId":15986,"journal":{"name":"Journal of Geophysical Research: Atmospheres","volume":"130 23","pages":""},"PeriodicalIF":3.4,"publicationDate":"2025-12-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2025JD043989","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145695228","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
The middle atmosphere circulation in the Korean Integrated Model (KIM) was evaluated at various horizontal resolutions and integration timescales. It was found that the intensities of the polar night jet and summer hemisphere easterly jet are underestimated. Consistent with the zonal wind, a warm (cold) bias in the mesosphere was found in the winter (summer) hemisphere high latitudes. This suggests that the gravity wave drag (GWD) is generally overestimated in KIM. The GWD in the mesosphere is dominated by the frontal GWD in the present simulations. In the frontal GWD parameterization, it was found that waves are launched more frequently and over a wider area at higher horizontal resolutions. To prevent the excessive generation of frontal gravity waves in the parameterization, the frontogenesis threshold used to diagnose the wave-launching region was revised. Instead of a constant threshold across different resolutions, the threshold value was modified to depend on the horizontal grid size so that wave regions are diagnosed similarly regardless of the horizontal resolution. Using a modified threshold decreases the GWD, which induces mesospheric cooling (warming) in the winter (summer) hemisphere high latitudes. As a result, the biases are alleviated in the mesosphere. The responses are extended to the lower stratosphere over an extended medium-range timescale. Lower stratospheric biases are reduced overall, but increase slightly in winter. Since the GWD is reduced to a greater degree at higher resolutions, biases are less reduced at lower resolutions, suggesting that the parameters for scale awareness in the GWD parameterization require further revisions.
{"title":"Effects of Resolution-Dependent Excitation of Parameterized Frontal Gravity Waves on the Middle Atmosphere Circulation in the Korean Integrated Model","authors":"So-Young Kim","doi":"10.1029/2025JD044822","DOIUrl":"https://doi.org/10.1029/2025JD044822","url":null,"abstract":"<p>The middle atmosphere circulation in the Korean Integrated Model (KIM) was evaluated at various horizontal resolutions and integration timescales. It was found that the intensities of the polar night jet and summer hemisphere easterly jet are underestimated. Consistent with the zonal wind, a warm (cold) bias in the mesosphere was found in the winter (summer) hemisphere high latitudes. This suggests that the gravity wave drag (GWD) is generally overestimated in KIM. The GWD in the mesosphere is dominated by the frontal GWD in the present simulations. In the frontal GWD parameterization, it was found that waves are launched more frequently and over a wider area at higher horizontal resolutions. To prevent the excessive generation of frontal gravity waves in the parameterization, the frontogenesis threshold used to diagnose the wave-launching region was revised. Instead of a constant threshold across different resolutions, the threshold value was modified to depend on the horizontal grid size so that wave regions are diagnosed similarly regardless of the horizontal resolution. Using a modified threshold decreases the GWD, which induces mesospheric cooling (warming) in the winter (summer) hemisphere high latitudes. As a result, the biases are alleviated in the mesosphere. The responses are extended to the lower stratosphere over an extended medium-range timescale. Lower stratospheric biases are reduced overall, but increase slightly in winter. Since the GWD is reduced to a greater degree at higher resolutions, biases are less reduced at lower resolutions, suggesting that the parameters for scale awareness in the GWD parameterization require further revisions.</p>","PeriodicalId":15986,"journal":{"name":"Journal of Geophysical Research: Atmospheres","volume":"130 23","pages":""},"PeriodicalIF":3.4,"publicationDate":"2025-12-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145694981","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Jianfei Liu, Wenjie Sun, Guozhu Li, Lianhuan Hu, Yi Li, Haiyong Xie, Xiukuan Zhao, Guofeng Dai, Baiqi Ning
Thunderstorm-related activities in the lower atmosphere are usually observed and investigated based on atmospheric weather radars. In this study, the occurrence of thunderstorms has been observed and investigated for the first time by all-sky meteor radars, which are primarily employed in mesospheric/ionospheric observations. By applying the radar interferometry technique to a bi-static all-sky radar system installed on Hainan Island, China, the thunderstorm activities on 5 June 2024 were captured and tracked. The thunderstorm echoes occurred at the altitudes ∼5–20 km along the southern coast of Hainan Island, lasted for ∼2 hr, and migrated northeastward at a speed of ∼15 m/s. The occurrence time, spatial locations in both the horizontal and vertical planes, and evolution of the echoes all corresponded well with the thunderstorm development process confirmed by multiple other kinds of lower-atmospheric observations. The study highlights the extended capability of all-sky radars in investigating lower-atmospheric activities, i.e., thunderstorms, which may favor the investigation on tropospheric-ionospheric coupling process during extreme convective activities in the future.
{"title":"First Observation of Thunderstorm Occurrences in the Lower Atmosphere by All-Sky Meteor Radars","authors":"Jianfei Liu, Wenjie Sun, Guozhu Li, Lianhuan Hu, Yi Li, Haiyong Xie, Xiukuan Zhao, Guofeng Dai, Baiqi Ning","doi":"10.1029/2025JD044232","DOIUrl":"https://doi.org/10.1029/2025JD044232","url":null,"abstract":"<p>Thunderstorm-related activities in the lower atmosphere are usually observed and investigated based on atmospheric weather radars. In this study, the occurrence of thunderstorms has been observed and investigated for the first time by all-sky meteor radars, which are primarily employed in mesospheric/ionospheric observations. By applying the radar interferometry technique to a bi-static all-sky radar system installed on Hainan Island, China, the thunderstorm activities on 5 June 2024 were captured and tracked. The thunderstorm echoes occurred at the altitudes ∼5–20 km along the southern coast of Hainan Island, lasted for ∼2 hr, and migrated northeastward at a speed of ∼15 m/s. The occurrence time, spatial locations in both the horizontal and vertical planes, and evolution of the echoes all corresponded well with the thunderstorm development process confirmed by multiple other kinds of lower-atmospheric observations. The study highlights the extended capability of all-sky radars in investigating lower-atmospheric activities, i.e., thunderstorms, which may favor the investigation on tropospheric-ionospheric coupling process during extreme convective activities in the future.</p>","PeriodicalId":15986,"journal":{"name":"Journal of Geophysical Research: Atmospheres","volume":"130 23","pages":""},"PeriodicalIF":3.4,"publicationDate":"2025-12-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145695076","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
This study analyzes the thermodynamic effects of atmospheric vertical motion recorded in satellite observations to investigate the processes behind the evolution of tropical convection. These processes, difficult to observe directly, are diagnosed from satellite retrievals of precipitation (P) and atmospheric cloud radiative effect (ACRE) with the aid of a simple theory. It is found that hourly changes of P and ACRE projected onto the P-ACRE plane have a tendency of pointing toward a settling point at LP