Solar Activity Continues to Rise with 'Anemone' Eruption
Short video showing the solar flare and subsequent prominence eruption and "arcade" of loops.
Credit: NASA/GSFC/SDO
Music: "Beautiful Awesome" from Universal Production Music
Watch this video on the NASA Goddard YouTube channel.
Complete transcript available.
This imagery captured by NASA’s Solar Dynamics Observatory shows a solar flare and a subsequent eruption of solar material that occurred over the left limb of the Sun on November 29, 2020. From its foot point over the limb, some of the light and energy was blocked from reaching Earth – a little like seeing light from a lightbulb with the bottom half covered up.
Also visible in the imagery is an eruption of solar material that achieved escape velocity and moved out into space as a giant cloud of gas and magnetic fields known as a coronal mass ejection, or CME. A third, but invisible, feature of such eruptive events also blew off the Sun: a swarm of fast-moving solar energetic particles. Such particles are guided by the magnetic fields streaming out from the Sun, which, due to the Sun’s constant rotation, point backwards in a big spiral much the way water comes out of a spinning sprinkler. The solar energetic particles, therefore, emerging as they did from a part of the Sun not yet completely rotated into our view, traveled along that magnetic spiral away from Earth toward the other side of the Sun.
While the solar material didn’t head toward Earth, it did pass by some spacecraft: NASA’s Parker Solar Probe, NASA’s STEREO and ESA/NASA’s Solar Orbiter. Equipped to measure magnetic fields and the particles that pass over them, we may be able to study fast-moving solar energetic particles in the observations once they are downloaded. These sun-watching missions are all part of a larger heliophysics fleet that help us understand both what causes such eruptions on the Sun -- as well as how solar activity affects interplanetary space, including near Earth, where they have the potential to affect astronauts and satellites.
A bright arcade of loops forms on the Sun on November 29, 2020. This image shows the structure in three wavelengths of light that highlight different parts of the structure.
Credit: NASA/GSFC/SDO
A prominence erupts from the Sun on November 29, 2020. This image shows the structure in three wavelengths of light that highlight different parts of the structure.
Credit: NASA/GSFC/SDO
Animated gif of solar activity from November 29, 2020. Captured by the Solar Dynamics Observatory in 131 angstrom light, this imagery highlights material at 12 million Kelvin.
Credit: NASA/GSFC/SDO
A beautiful arcade of loops forms on the Sun on November 29, 2020. This image was captured by NASA's Solar Dynamics Observatory and shows a blend of light in the 171 and 131 angstrom wavelength.
Credit: NASA/GSFC/SDO
The Sun on November 29, 2020. This image was captured by NASA's Solar Dynamics Observatory and shows light in the 171 angstrom wavelength.
Credit: NASA/GSFC/SDO
4k frames and video covering a time period of 11:00 UT on November 29 to 09:00 UT on November 30, 2020. 131 angstrom wavelength extreme ultraviolet light.
Credit: NASA/GSFC/SDO
4k frames and video covering a time period of 11:00 UT on November 29 to 09:00 UT on November 30, 2020. 171 angstrom wavelength extreme ultraviolet light.
Credit: NASA/GSFC/SDO
4k frames and video covering a time period of 11:00 UT on November 29 to 09:00 UT on November 30, 2020. 304 angstrom wavelength extreme ultraviolet light.
Credit: NASA/GSFC/SDO
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Credits
Please give credit for this item to:
NASA's Goddard Space Flight Center. However, individual items should be credited as indicated above.
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Producer
- Scott Wiessinger (USRA)
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Visualizer
- Tom Bridgman (Global Science and Technology, Inc.)
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Science writers
- Karen Fox (ADNET Systems, Inc.)
- Miles S. Hatfield (Telophase)
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Video editor
- Scott Wiessinger (USRA)
Release date
This page was originally published on Thursday, December 3, 2020.
This page was last updated on Wednesday, May 3, 2023 at 1:44 PM EDT.