Electron acceleration and transport in the 2023-03-06 solar flare
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arXiv
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| Autori principali: | , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2024
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| _version_ | 1866909212702932992 |
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| author | Kuznetsov, Alexey Wu, Zhao Anfinogentov, Sergey Su, Yang Chen, Yao |
| author_facet | Kuznetsov, Alexey Wu, Zhao Anfinogentov, Sergey Su, Yang Chen, Yao |
| contents | We investigated in detail the M5.8 class solar flare that occurred on 2023-03-06. This flare was one of the first strong flares observed by the Siberian Radioheliograph in the microwave range and the Advanced Space-based Solar Observatory in the X-ray range. The flare consisted of two separate flaring events (a "thermal" and a "cooler" ones), and was associated with (and probably triggered by) a filament eruption. During the first part of the flare, the microwave emission was produced in an arcade of relatively short and low flaring loops. During the second part of the flare, the microwave emission was produced by energetic electrons trapped near the top of a large-scale flaring loop; the evolution of the trapped electrons was mostly affected by the Coulomb collisions. Using the available observations and the GX Simulator tool, we created a 3D model of the flare, and estimated the parameters of the energetic electrons in it. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2405_18850 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Electron acceleration and transport in the 2023-03-06 solar flare Kuznetsov, Alexey Wu, Zhao Anfinogentov, Sergey Su, Yang Chen, Yao Solar and Stellar Astrophysics We investigated in detail the M5.8 class solar flare that occurred on 2023-03-06. This flare was one of the first strong flares observed by the Siberian Radioheliograph in the microwave range and the Advanced Space-based Solar Observatory in the X-ray range. The flare consisted of two separate flaring events (a "thermal" and a "cooler" ones), and was associated with (and probably triggered by) a filament eruption. During the first part of the flare, the microwave emission was produced in an arcade of relatively short and low flaring loops. During the second part of the flare, the microwave emission was produced by energetic electrons trapped near the top of a large-scale flaring loop; the evolution of the trapped electrons was mostly affected by the Coulomb collisions. Using the available observations and the GX Simulator tool, we created a 3D model of the flare, and estimated the parameters of the energetic electrons in it. |
| title | Electron acceleration and transport in the 2023-03-06 solar flare |
| topic | Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2405.18850 |