What are solar prominences and are they the same as solar flares?
nbcdfw.com
What are solar prominences and are they the same as solar flares?
NBC 5 Meteorologist Kevan Smith explains the differences between solar prominences and solar flares.
Apr 10, 2024
Shorts
Solar Closeup and prominence Time Lapse on February 15, 2026. #science #space #solarimaging
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860 views
Solar Closeup and prominence Time Lapse on February 15, 2026. #science
Silverton Texas AstroBox
One of the coolest features seen during the total solar eclipse were the solar prominences! They were huge and bright! From @nasa - A solar prominence (also known as a filament when viewed against the solar disk) is a large, bright feature extending outward from the Sun’s surface. Prominences are anchored to the Sun’s surface in the photosphere, and extend outwards into the Sun’s hot outer atmosphere, called the corona. A prominence forms over timescales of about a day, and stable prominences ma
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146.5K views
One of the coolest features seen during the total solar eclipse were the solar
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Top videos
What are solar prominences and are they the same as solar flares?
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What are solar prominences and are they the same as solar flares?
YouTubeNBC DFW
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🔴 Incredible Solar Flare, Prominence Eruption and CME Event (304 angstroms) 15.7.2019 • On June 7, 2011, an M-2 flare occurred on the Sun which released a very large coronal mass ejection (CME). Much of the ejected material is much cooler (less than about 80,000K) and therefore appears dark against the brighter solar disk. Material which does not reach solar escape velocity can be seen falling back and striking the solar surface, sometimes triggering smaller events. This image sequence is captu
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🔴 Incredible Solar Flare, Prominence Eruption and CME Event (304 angstroms) 15.7.2019 • On June 7, 2011, an M-2 flare occurred on the Sun which released a very large coronal mass ejection (CME). Much of the ejected material is much cooler (less than about 80,000K) and therefore appears dark against the brighter solar disk. Material which does not reach solar escape velocity can be seen falling back and striking the solar surface, sometimes triggering smaller events. This image sequence is captu
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The Sun emitted a strong solar flare on Dec. 14, 2023, peaking at 12:02 ET. NASA’s Solar Dynamics Observatory captured an image of the event, which was classified as X2.8. https://go.nasa.gov/3Ts3a1Q Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth’s atmosphere to physically affect humans on the ground. However – when intense enough – they can disturb the atmosphere in the layer where GPS & communications signals travel. To see how such spac
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The Sun emitted a strong solar flare on Dec. 14, 2023, peaking at 12:02 ET. NASA’s Solar Dynamics Observatory captured an image of the event, which was classified as X2.8. https://go.nasa.gov/3Ts3a1Q Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth’s atmosphere to physically affect humans on the ground. However – when intense enough – they can disturb the atmosphere in the layer where GPS & communications signals travel. To see how such spac
FacebookNASA Space Alerts
4.5K viewsDec 14, 2023
The Sun emitted a strong solar flare on Nov. 30, 2025, peaking at 9:49 p.m. ET. NASA’s Solar Dynamics Observatory captured an image of the event, which was classified as X1.9 class: go.nasa.gov/4alXf6P Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth’s atmosphere to physically affect humans on the ground. However — when intense enough — they can disturb the atmosphere in the layer where GPS & communications signals travel. To see how such sp
0:08
The Sun emitted a strong solar flare on Nov. 30, 2025, peaking at 9:49 p.m. ET. NASA’s Solar Dynamics Observatory captured an image of the event, which was classified as X1.9 class: go.nasa.gov/4alXf6P Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth’s atmosphere to physically affect humans on the ground. However — when intense enough — they can disturb the atmosphere in the layer where GPS & communications signals travel. To see how such sp
FacebookNASA Space Alerts
25K views5 months ago
The Sun emitted a strong solar flare on Jan. 5, 2023, peaking at 7:57 p.m. ET. NASA’s Solar Dynamics Observatory captured an image of the event, which was classified as X-class. bit.ly/3IsPJsW Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth’s atmosphere to physically affect humans on the ground, however – when intense enough – they can disturb the atmosphere in the layer where GPS & communications signals travel. To see how such space weath
0:11
The Sun emitted a strong solar flare on Jan. 5, 2023, peaking at 7:57 p.m. ET. NASA’s Solar Dynamics Observatory captured an image of the event, which was classified as X-class. bit.ly/3IsPJsW Solar flares are powerful bursts of radiation. Harmful radiation from a flare cannot pass through Earth’s atmosphere to physically affect humans on the ground, however – when intense enough – they can disturb the atmosphere in the layer where GPS & communications signals travel. To see how such space weath
FacebookNASA Space Alerts
2.7K viewsJan 6, 2023
What are solar prominences and are they the same as solar flares?
1:21
What are solar prominences and are they the same as solar flares?
1K viewsApr 10, 2024
YouTubeNBC DFW
🔴 Incredible Solar Flare, Prominence Eruption and CME Event (304 angstroms) 15.7.2019 • On June 7, 2011, an M-2 flare occurred on the Sun which released a very large coronal mass ejection (CME). Much of the ejected material is much cooler (less than about 80,000K) and therefore appears dark against the brighter solar disk. Material which does not reach solar escape velocity can be seen falling back and striking the solar surface, sometimes triggering smaller events. This image sequence is captu
0:14
🔴 Incredible Solar Flare, Prominence Eruption and CME Event (304 angstroms) 15.7.2019 • On June 7, 2011, an M-2 flare occurred on the Sun which released a very large coronal mass ejection (CME). Much of the ejected material is much cooler (less than about 80,000K) and therefore appears dark against the brighter solar disk. Material which does not reach solar escape velocity can be seen falling back and striking the solar surface, sometimes triggering smaller events. This image sequence is captu
2.9K viewsJul 15, 2019
FacebookAstronomy Nation
Prominences, Solar Flares and Sun Spots
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Prominences, Solar Flares and Sun Spots
12.4K viewsJan 26, 2012
YouTubeRegion 10 ESC
• A Prominence Eruption with a M-class Solar Flare • We can see prominence erupting to interplanetary space. A flare occurs simultaneously at the bottom region of the eruption. (Observed by Solar Optical Telescope (SOT), wavelength: calcium H line [396 nm]) [Instrument: Hinode/ Solar Optical Telescope (SOT), Wavelength: 394 nm Calcium H line)] Occurred on 16 April 2012. • Credit: “NAOJ, JAXA, NASA/MSFC” | Astronomy Nation
0:19
• A Prominence Eruption with a M-class Solar Flare • We can see prominence erupting to interplanetary space. A flare occurs simultaneously at the bottom region of the eruption. (Observed by Solar Optical Telescope (SOT), wavelength: calcium H line [396 nm]) [Instrument: Hinode/ Solar Optical Telescope (SOT), Wavelength: 394 nm Calcium H line)] Occurred on 16 April 2012. • Credit: “NAOJ, JAXA, NASA/MSFC” | Astronomy Nation
124.3K views5 months ago
FacebookAstronomy Nation
Solar Phenomena | Solar Prominences, Solar Flares & Coronal Mass Ejections
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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
1.7K viewsOct 14, 2022
FacebookCanadian Space Agency
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Solar Prominence by Hinode Solar prominence is cool gas floating in the solar atmosphere. Prominence material is denser than surrounding coronal plasma, but it is sometimes suspended in the corona for a long time. Coronal magnetic fields could act like a hammock, supporting the prominence material. Gas in the prominence moves up and down, showing the waves are propagating along magnetic field lines. It is thought that this wave may carry energy from the photosphere to the corona and that the ene
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FacebookAstronomy Nation
Is a solar flare the same thing as a CME?
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One of the coolest features seen during the total solar eclipse were the solar prominences! They were huge and bright! From @nasa - A solar prominence (also known as a filament when viewed against the solar disk) is a large, bright feature extending outward from the Sun’s surface. Prominences are anchored to the Sun’s surface in the photosphere, and extend outwards into the Sun’s hot outer atmosphere, called the corona. A prominence forms over timescales of about a day, and stable prominences ma
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A Phoenix prominence eruption on the sun
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