Global distribution of key features of streamer corona discharges in thunderclouds
| العنوان: | Global distribution of key features of streamer corona discharges in thunderclouds |
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| المؤلفون: | S. Soler, F. J. Gordillo‐Vázquez, F. J. Pérez‐Invernón, A. Luque, D. Li, T. Neubert, O. Chanrion, V. Reglero, J. Navarro‐González, N. Østgaard |
| المساهمون: | Ministerio de Ciencia e Innovación (España), European Commission, European Research Council |
| المصدر: | Soler, S, Gordillo-Vázquez, F J, Pérez-Invernón, F J, Luque, A, Li, D, Neubert, T, Chanrion, O, Reglero, V, Navarro-González, J & Østgaard, N 2022, ' Global distribution of key features of streamer corona discharges in thunderclouds ', Journal of Geophysical Research: Atmospheres, vol. 127, e2022JD037535 . https://doi.org/10.1029/2022JD037535 e2022JD037535 Journal of Geophysical Research (JGR): Atmospheres |
| سنة النشر: | 2022 |
| مصطلحات موضوعية: | Remote Sensing, Atmospheric Science, Geophysics, Corona discharges in thunderclouds, Space and Planetary Science, Earth and Planetary Sciences (miscellaneous), Remote sensing, Lightning, ASIM |
| الوصف: | This is an open access article under the terms of the Creative Commons Attribution-NonCommercial License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited and is not used for commercial purposes. We present nighttime worldwide distributions of key features of Blue LUminous Events (BLUEs) detected by the Modular Multispectral Imaging Array of the Atmosphere-Space Interaction Monitor. Around 10% of all detected BLUEs exhibit an impulsive single pulse shape. The rest of BLUEs are unclear (impulsive or not) single, multiple or with ambiguous pulse shapes. BLUEs exhibit two distinct populations with peak power density ASIM is a mission of ESA's SciSpace programme for scientific utilization of the ISS and non-ISS space exploration platforms and space environment analogues. ASIM and the ASIM Science Data Centre are funded by ESA and by national grants of Denmark, Norway, and Spain. This work was supported by the Spanish Ministry of Science and Innovation under project PID2019-109269RB-C43 and the FEDER program. SS acknowledges a PhD research contract through the project PID2019-109269RB-C43. FJPI acknowledges the sponsorship provided by Junta de Andalucía under Grant POSTDOC-21-00052. AL and DL were supported by the European Research Council (ERC) under European Union H2020 programme/ERC grant agreement 681257. SS, FJGV, AL, and DL acknowledge financial support from the State Agency for Research of the Spanish MCIU through the ”Center of Excellence Severo Ochoa” award for the Instituto de Astrofísica de Andalucía (SEV-2017-0709). |
| وصف الملف: | application/pdf |
| اللغة: | English |
| DOI: | 10.1029/2022JD037535 |
| URL الوصول: | https://explore.openaire.eu/search/publication?articleId=doi_dedup___::92222d3623a0fec37282764480a11fa1 https://orbit.dtu.dk/en/publications/7d7303ad-777e-4e14-ae66-8fcb7aa89c78 |
| Rights: | OPEN |
| رقم الانضمام: | edsair.doi.dedup.....92222d3623a0fec37282764480a11fa1 |
| قاعدة البيانات: | OpenAIRE |
| DOI: | 10.1029/2022JD037535 |
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