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In solar physics, a coronal loop is an ill-defined arch-like structure in the Sun's atmosphere made up of relatively dense plasma confined and isolated from the surrounding medium by magnetic flux tubes. Coronal loops begin and end at two footpoints on the photosphere and project into the transition region and lower corona. They typically form and…
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coronal solar loops magnetic plasma corona loop surface photosphere active field sun's transition region observations trace soho flux cycle range
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Coronal loop | is a | ill-defined arch-like structure in the Sun's atmosphere made up of relatively dense plasma confined and isolated from the surrounding medium by magnetic flux tubes | 0.90 | text |
| the Aerobee flights | instance of | Rocket missions | 0.80 | text |
| Skylark rockets successfully measured solar extreme ultraviolet | instance of | Rocket missions | 0.80 | text |
| the Orbiting Solar Observatory series | instance of | satellites | 0.80 | text |
| Coronal loop | related to 1991–present day | In August | 0.60 | section |
| Coronal loop | related to 1991–present day | Yohkoh | 0.60 | section |
| Coronal loop | related to 1991–present day | Kagoshima Space Center | 0.60 | section |
| Coronal loop | related to 1991–present day | During | 0.60 | section |
| Coronal loop | related to 1991–present day | X-ray | 0.60 | section |
| Coronal loop | related to 1991–present day | SXT | 0.60 | section |
| Coronal loop | related to 1991–present day | X-ray-emitting | 0.60 | section |
| Coronal loop | related to 1991–present day | This | 0.60 | section |
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