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?
NBC 5 Meteorologist Kevan Smith explains the differences between solar prominences and solar flares.
Apr 10, 2024
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Solar Closeup and prominence Time Lapse on February 15, 2026. #science #space #solarimaging
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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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One of the coolest features seen during the total solar eclipse were the solar
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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?
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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
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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
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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
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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
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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
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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?
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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
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• 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
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