Suppression of ion heating in the cusp during plasma flow burst
Abstract Previous studies have shown the occurrence of short-duration plasma flow bursts, typically lasting a few minutes, within the cusp region, often accompanied by the poleward motion of the 630-nm aurora. In this study, we investigated the ion heating characteristics associated with a large-sca...
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| Format: | Article |
| Language: | English |
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SpringerOpen
2025-08-01
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| Series: | Earth, Planets and Space |
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| Online Access: | https://doi.org/10.1186/s40623-025-02264-z |
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| author | Satoshi Taguchi Tomokazu Oigawa Yunosuke Nagafusa Hiroyuki Shinagawa Keisuke Hosokawa Yasunobu Ogawa Haruto Koike |
| author_facet | Satoshi Taguchi Tomokazu Oigawa Yunosuke Nagafusa Hiroyuki Shinagawa Keisuke Hosokawa Yasunobu Ogawa Haruto Koike |
| author_sort | Satoshi Taguchi |
| collection | DOAJ |
| description | Abstract Previous studies have shown the occurrence of short-duration plasma flow bursts, typically lasting a few minutes, within the cusp region, often accompanied by the poleward motion of the 630-nm aurora. In this study, we investigated the ion heating characteristics associated with a large-scale plasma flow burst, which coincides with a poleward expansion of the 630-nm aurora. We analyzed data from simultaneous observations using an all-sky imager at Svalbard, the EISCAT Svalbard Radar (ESR), and the SuperDARN radar at Hankasalmi. Additionally, we examined magnetic perturbation data from the Swarm satellites as complementary data to assess the presence of a significant east–west component in the plasma flow. The plasma flow burst was detected by the ESR at approximately 10:40 UT on 8 December 2016, indicated by an increase in the F-region ion temperature ( $${T}_{i}$$ T i ) due to frictional heating arising from ion–neutral velocity differences. Coinciding with the arrival of the front of the plasma flow burst within the ESR’s field of view (accurate to within 1 min), the poleward boundary of the cusp electron precipitation, as observed in the 630-nm aurora, passed through the ESR’s field of view by moving poleward, seemingly drawn by the front of the plasma flow burst. The altitude profiles of $${T}_{i}$$ T i revealed a local maximum at an altitude of approximately 150 km, where the temperature increased from ~ 1200 to ~ 1880 K within 4 min. At altitudes between 190 and 300 km $${T}_{i}$$ T i was lower than this local maximum $${T}_{i}$$ T i prior to the plasma flow burst, but rapidly increased to approximately match the local maximum $${T}_{i}$$ T i . However, following this rapid increase, the $${T}_{i}$$ T i enhancement at these altitudes appeared to be suppressed, with the estimated rate of suppression being −80 and −220 K/min. Based on the investigation through two-dimensional simplified numerical simulations, we suggest that the suppression of $${T}_{i}$$ T i is likely due to the formation of a relatively fast neutral flow, driven by increased ion drag associated with ionization enhancement resulting from low-energy electron precipitation. Graphical Abstract |
| format | Article |
| id | doaj-art-2e4bd9a61c3e4e13a9e50a05e54ec0fa |
| institution | Kabale University |
| issn | 1880-5981 |
| language | English |
| publishDate | 2025-08-01 |
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| series | Earth, Planets and Space |
| spelling | doaj-art-2e4bd9a61c3e4e13a9e50a05e54ec0fa2025-08-20T03:47:10ZengSpringerOpenEarth, Planets and Space1880-59812025-08-0177112010.1186/s40623-025-02264-zSuppression of ion heating in the cusp during plasma flow burstSatoshi Taguchi0Tomokazu Oigawa1Yunosuke Nagafusa2Hiroyuki Shinagawa3Keisuke Hosokawa4Yasunobu Ogawa5Haruto Koike6Department of Geophysics, Graduate School of Science, Kyoto UniversityDepartment of Geophysics, Graduate School of Science, Kyoto UniversityDepartment of Geophysics, Graduate School of Science, Kyoto UniversityInternational Research Center for Space and Planetary Environmental Science, Kyushu UniversityGraduate School of Communication Engineering and Informatics, and Center for Space Science and Radio Engineering, University of Electro-CommunicationsNational Institute of Polar ResearchDepartment of Geophysics, Graduate School of Science, Kyoto UniversityAbstract Previous studies have shown the occurrence of short-duration plasma flow bursts, typically lasting a few minutes, within the cusp region, often accompanied by the poleward motion of the 630-nm aurora. In this study, we investigated the ion heating characteristics associated with a large-scale plasma flow burst, which coincides with a poleward expansion of the 630-nm aurora. We analyzed data from simultaneous observations using an all-sky imager at Svalbard, the EISCAT Svalbard Radar (ESR), and the SuperDARN radar at Hankasalmi. Additionally, we examined magnetic perturbation data from the Swarm satellites as complementary data to assess the presence of a significant east–west component in the plasma flow. The plasma flow burst was detected by the ESR at approximately 10:40 UT on 8 December 2016, indicated by an increase in the F-region ion temperature ( $${T}_{i}$$ T i ) due to frictional heating arising from ion–neutral velocity differences. Coinciding with the arrival of the front of the plasma flow burst within the ESR’s field of view (accurate to within 1 min), the poleward boundary of the cusp electron precipitation, as observed in the 630-nm aurora, passed through the ESR’s field of view by moving poleward, seemingly drawn by the front of the plasma flow burst. The altitude profiles of $${T}_{i}$$ T i revealed a local maximum at an altitude of approximately 150 km, where the temperature increased from ~ 1200 to ~ 1880 K within 4 min. At altitudes between 190 and 300 km $${T}_{i}$$ T i was lower than this local maximum $${T}_{i}$$ T i prior to the plasma flow burst, but rapidly increased to approximately match the local maximum $${T}_{i}$$ T i . However, following this rapid increase, the $${T}_{i}$$ T i enhancement at these altitudes appeared to be suppressed, with the estimated rate of suppression being −80 and −220 K/min. Based on the investigation through two-dimensional simplified numerical simulations, we suggest that the suppression of $${T}_{i}$$ T i is likely due to the formation of a relatively fast neutral flow, driven by increased ion drag associated with ionization enhancement resulting from low-energy electron precipitation. Graphical Abstracthttps://doi.org/10.1186/s40623-025-02264-zCuspPlasma flow burstIon heatingIon dragAuroraElectron precipitation |
| spellingShingle | Satoshi Taguchi Tomokazu Oigawa Yunosuke Nagafusa Hiroyuki Shinagawa Keisuke Hosokawa Yasunobu Ogawa Haruto Koike Suppression of ion heating in the cusp during plasma flow burst Earth, Planets and Space Cusp Plasma flow burst Ion heating Ion drag Aurora Electron precipitation |
| title | Suppression of ion heating in the cusp during plasma flow burst |
| title_full | Suppression of ion heating in the cusp during plasma flow burst |
| title_fullStr | Suppression of ion heating in the cusp during plasma flow burst |
| title_full_unstemmed | Suppression of ion heating in the cusp during plasma flow burst |
| title_short | Suppression of ion heating in the cusp during plasma flow burst |
| title_sort | suppression of ion heating in the cusp during plasma flow burst |
| topic | Cusp Plasma flow burst Ion heating Ion drag Aurora Electron precipitation |
| url | https://doi.org/10.1186/s40623-025-02264-z |
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