Intense Geomagnetic Storms during Solar Cycles 23-25
Fuente:
arXiv
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| Autori principali: | , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2024
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| _version_ | 1866914633766404096 |
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| author | Gopalswamy, N. Akiyama, S. Yashiro, S. Makela, P. Xie, H. |
| author_facet | Gopalswamy, N. Akiyama, S. Yashiro, S. Makela, P. Xie, H. |
| contents | Intense geomagnetic storms are characterized by a minimum value of the Dst index at or below -100 nT. It is well known that these storms are caused by the southward magnetic fields in coronal mass ejections (CMEs) and corotating interaction regions (CIRs). While CIR storms are confined to Dst values at or above -150 nT, CME storms can reach Dst -500 nT or lower. In this report, we illustrate the need to understand the storm evolution based on solar source and solar wind parameters using a recent storm (2023 April 24) by way of providing the motivation to catalog such events for a better understanding of the main phase time structure of geomagnetic storms |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2401_03524 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Intense Geomagnetic Storms during Solar Cycles 23-25 Gopalswamy, N. Akiyama, S. Yashiro, S. Makela, P. Xie, H. Solar and Stellar Astrophysics Space Physics Intense geomagnetic storms are characterized by a minimum value of the Dst index at or below -100 nT. It is well known that these storms are caused by the southward magnetic fields in coronal mass ejections (CMEs) and corotating interaction regions (CIRs). While CIR storms are confined to Dst values at or above -150 nT, CME storms can reach Dst -500 nT or lower. In this report, we illustrate the need to understand the storm evolution based on solar source and solar wind parameters using a recent storm (2023 April 24) by way of providing the motivation to catalog such events for a better understanding of the main phase time structure of geomagnetic storms |
| title | Intense Geomagnetic Storms during Solar Cycles 23-25 |
| topic | Solar and Stellar Astrophysics Space Physics |
| url | https://arxiv.org/abs/2401.03524 |