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M-Class Solar Flares in Solar Cycles 23 and 24: Properties and Space Weather Relevance
| Content Provider | MDPI |
|---|---|
| Author | Miteva, Rositsa Samwel, Susan W. |
| Copyright Year | 2022 |
| Abstract | A comprehensive statistical analysis on the properties and accompanied phenomena of all M-class solar flares (as measured in soft X-rays) in the last two solar cycles (1996–2019) is presented here with a focus on their space weather potential. The information about the parent active region and the underlying sunspot (Hale) type is collected for each case, where possible, in order to identify photospheric precondition as precursors for the solar flare eruption or confinement. Associations with coronal mass ejections, solar energetic particles, and interplanetary radio emissions are also evaluated and discussed as possible proxies for flare eruption and subsequent space weather relevance. The results show that the majority (∼80%) of the analyzed M-class flares are of |
| Starting Page | 39 |
| e-ISSN | 22181997 |
| DOI | 10.3390/universe8010039 |
| Journal | Universe |
| Issue Number | 1 |
| Volume Number | 8 |
| Language | English |
| Publisher | MDPI |
| Publisher Date | 2022-01-10 |
| Access Restriction | Open |
| Subject Keyword | Universe Astronomy and Astrophysics Space Weather Solar Flares Coronal Mass Ejections Solar Radio Bursts Solar Energetic Particles |
| Content Type | Text |
| Resource Type | Article |