Solar prominences, solar flares, chromosphere, corona | Britannica
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britannica.com
Solar prominences, solar flares, chromosphere, corona | Britannica
Prominences are clouds of incandescent, ionized gas ejected from the Sun's surface. They are also some of the most dramatic phenomena in the solar system, the equivalent of thousand-mile-high storms that can rage for months. This time-lapse film shows active prominences of a few hours' duration. “Loop” prominences like this one, which seems ...
Feb 24, 2020
Solar prominence Formation
1.7K views · 130 reactions | A large eruption occurs off the limb of the Sun in this image sequence, and you can see the solar prominence in the lower right. ☀️ Prominences appear when relatively cooler gas from lower layers of the Sun’s atmosphere is trapped in a magnetic field loop that extends outward from the Sun’s surface, into the hotter corona. Video: NASA | Canadian Space Agency | Facebook
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1.7K views · 130 reactions | A large eruption occurs off the limb of the Sun in this image sequence, and you can see the solar prominence in the lower right. ☀️ Prominences appear when relatively cooler gas from lower layers of the Sun’s atmosphere is trapped in a magnetic field loop that extends outward from the Sun’s surface, into the hotter corona. Video: NASA | Canadian Space Agency | Facebook
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Giant Hummingbird Solar Prominence Captured by James Sinclair #sun #space #astronomy #astrophotography | Nikola Sagan
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Space | Cosmos | Galaxy on Instagram: "A Solar Prominence is a large, bright, looped feature of plasma extending from the Sun's surface into the corona, held in place by magnetic fields. These structures can be hundreds of thousands of miles long and may last for days or months, but if they become unstable, they can erupt and release plasma into space. Credits: @simon2940"
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Space | Cosmos | Galaxy on Instagram: "A Solar Prominence is a large, bright, looped feature of plasma extending from the Sun's surface into the corona, held in place by magnetic fields. These structures can be hundreds of thousands of miles long and may last for days or months, but if they become unstable, they can erupt and release plasma into space. Credits: @simon2940"
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• Through the Hoops • A dark prominence can be seen crossing right underneath a coronal loop as they both rotate into view (Aug. 26 - 28, 2012). Prominences are long strands of cooler gases that float above the Sun's surface. The loops that we see here in extreme ultraviolet light are magnetic field lines being traced by spiraling particles above active regions. It is not uncommon for a prominence to stretch under these connecting loops, but it is harder to see unless they are in profile, as the
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• Through the Hoops • A dark prominence can be seen crossing right underneath a coronal loop as they both rotate into view (Aug. 26 - 28, 2012). Prominences are long strands of cooler gases that float above the Sun's surface. The loops that we see here in extreme ultraviolet light are magnetic field lines being traced by spiraling particles above active regions. It is not uncommon for a prominence to stretch under these connecting loops, but it is harder to see unless they are in profile, as the
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Space | Cosmos | Galaxy on Instagram: "A Solar Prominence is a large, bright, looped feature of plasma extending from the Sun's surface into the corona, held in place by magnetic fields. These structures can be hundreds of thousands of miles long and may last for days or months, but if they become unstable, they can erupt and release plasma into space. Credits: @simon2940"
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• Through the Hoops • A dark prominence can be seen crossing right underneath a coronal loop as they both rotate into view (Aug. 26 - 28, 2012). Prominences are long strands of cooler gases that float above the Sun's surface. The loops that we see here in extreme ultraviolet light are magnetic field lines being traced by spiraling particles above active regions. It is not uncommon for a prominence to stretch under these connecting loops, but it is harder to see unless they are in profile, as the
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1.7K views · 130 reactions | A large eruption occurs off the limb of the Sun in this image sequence, and you can see the solar prominence in the lower right. ☀️ Prominences appear when relatively cooler gas from lower layers of the Sun’s atmosphere is trapped in a magnetic field loop that extends outward from the Sun’s surface, into the hotter corona. Video: NASA | Canadian Space Agency | Facebook
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