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In solar physics, an active region is a temporary feature in the Sun's atmosphere characterized by a strong and complex magnetic field. Active regions are often associated with sunspots and are commonly the source of violent eruptions such as coronal mass ejections and solar flares. The number and location of active regions on the solar disk at any given…
Regions, Overview & Region numbers
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active solar regions magnetic region sunspots field persist upflow contains flows often number appear following complex relatively numbers mount wilson
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Active region | is a | temporary feature in the Sun's atmosphere characterized by a strong and complex magnetic field | 0.90 | text |
| coronal mass ejections | instance of | Active regions are often associated with sunspots and are commonly the source of violent eruptions | 0.80 | text |
| solar flares | instance of | Active regions are often associated with sunspots and are commonly the source of violent eruptions | 0.80 | text |
| Active region | related to Coronal Field Connectivity | The | 0.60 | section |
| Active region | related to Coronal Field Connectivity | In | 0.60 | section |
| Active region | related to Magnetic flux emergence | Active | 0.60 | section |
| Active region | related to Mount Wilson magnetic classification | The Mount Wilson | 0.60 | section |
| Active region | related to Mount Wilson magnetic classification | Hale | 0.60 | section |
| Active region | related to Mount Wilson magnetic classification | It | 0.60 | section |
| Active region | related to Mount Wilson magnetic classification | George Ellery Hale | 0.60 | section |
| Active region | related to Mount Wilson magnetic classification | Mount Wilson Observatory | 0.60 | section |
| Active region | related to Mount Wilson magnetic classification | Künzel | 0.60 | section |
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