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Sunspots are temporary spots on the Sun's surface that are darker than the surrounding area. They are regions of reduced surface temperature caused by concentrations of magnetic flux that inhibit convection. Sunspots appear within active regions, usually in pairs of opposite magnetic polarity. Their number varies according to the approximately 11-year…
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sunspots solar magnetic sun cycle photosphere activity numbers field active regions umbra number 000 surface minimum spots also data years
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| coronal loops | instance of | sunspots accompany other active region phenomena | 0.80 | text |
| prominences | instance of | sunspots accompany other active region phenomena | 0.80 | text |
| and reconnection events | instance of | sunspots accompany other active region phenomena | 0.80 | text |
| Richard Carrington in 1865 | instance of | Years later scientists | 0.80 | text |
| John Henry Poynting in 1884 tried | instance of | Years later scientists | 0.80 | text |
| failed to find a connection between wheat prices | instance of | Years later scientists | 0.80 | text |
| sunspots | instance of | Years later scientists | 0.80 | text |
| and modern analysis finds that there is no statistically significant correlation between wheat prices | instance of | Years later scientists | 0.80 | text |
| sunspot numbers | instance of | Years later scientists | 0.80 | text |
| spectroscopes | instance of | Specialized tools | 0.80 | text |
| spectrohelioscopes are used to examine sunspots | instance of | Specialized tools | 0.80 | text |
| sunspot areas | instance of | Specialized tools | 0.80 | text |
These clusters group vocabulary that occurs around closely connected concepts in the source material.
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