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"url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/New_Trebuchet_mkII.00300_print.jpg",
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"alt_text": "The Trebuchet eruption (upper left) as seen in the SDO AIA 304 angstrom filter. This is probably one of the more popular views of the event.4k source files",
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"alt_text": "The Trebuchet eruption (upper left) as seen in the SDO AIA 304 angstrom filter. This is probably one of the more popular views of the event.4k source files",
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"url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/New_Trebuchet_mkII.00300_print_thm.png",
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"url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/New_Trebuchet_mkII.mp4",
"filename": "New_Trebuchet_mkII.mp4",
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"alt_text": "The Trebuchet eruption (upper left) as seen in the SDO AIA 304 angstrom filter. This is probably one of the more popular views of the event.4k source files",
"width": 1920,
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"filename": "New_Trebuchet_mkII.webm",
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"alt_text": "The Trebuchet eruption (upper left) as seen in the SDO AIA 304 angstrom filter. This is probably one of the more popular views of the event.4k source files",
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"id": 213390,
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"id": 372188,
"url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/New_Trebuchet_mkII.mov",
"filename": "New_Trebuchet_mkII.mov",
"media_type": "Movie",
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"description": "These clips are elements from various solar videos produced by NASA's Goddard Space Flight Center. Use them to create your own artistic video with the Sun as its theme.
These shots are all 1920x1080, but they originate from imagery collected by the Solar Dynamics Observatory (SDO.) All of that is 4,096 x 4,096 pixels in size and shows the full solar disk. This source material is linked to in the description of each shot.",
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"description": "A moderate solar flare was emitted by the sun on July 19, 2012. At 5:58 UTC it peaked at M7.7 on the flare scale, which makes it fairly powerful, but still much weaker than X-class flares, which are the largest. What made this particular event so noteworthy was the associated activity in the sun's corona. For the next day, hot plasma in corona cooled and condensed along the strong magnetic fields of the region that produced the flare. Magnetic fields are invisible, but the plasma is very obvious in the extreme ultraviolet wavelength of 304 angstroms, which highlights material at a temperature of about 50,000 Kelvin. This plasma is attracted to the magnetic fields and outlines them very clearly as it slowly falls back to the solar surface. This process of condensing plasma falling to the surface is called coronal rain.
The footage in this video was collected by the Solar Dynamics Observatory's AIA instrument. SDO collected one frame every 12 seconds.
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This plasma is attracted to the magnetic fields and outlines them very clearly as it slowly falls back to the solar surface. This process of condensing plasma falling to the surface is called coronal rain.The footage in this video was collected by the Solar Dynamics Observatory's AIA instrument. SDO collected one frame every 12 seconds.4k source material", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 213398, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 372196, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/Helios_Second_Shot_MkIII.webm", "filename": "Helios_Second_Shot_MkIII.webm", "media_type": "Movie", "alt_text": "A moderate solar flare was emitted by the sun on July 19, 2012. At 5:58 UTC it peaked at M7.7 on the flare scale, which makes it fairly powerful, but still much weaker than X-class flares, which are the largest. What made this particular event so noteworthy was the associated activity in the sun's corona. For the next day, hot plasma in corona cooled and condensed along the strong magnetic fields of the region that produced the flare. Magnetic fields are invisible, but the plasma is very obvious in the extreme ultraviolet wavelength of 304 angstroms, which highlights material at a temperature of about 50,000 Kelvin. This plasma is attracted to the magnetic fields and outlines them very clearly as it slowly falls back to the solar surface. This process of condensing plasma falling to the surface is called coronal rain.The footage in this video was collected by the Solar Dynamics Observatory's AIA instrument. 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SDO collected one frame every 12 seconds.4k source material", "width": 1920, "height": 1080, "pixels": 2073600 } } ], "extra_data": {} }, { "id": 314975, "url": "https://svs.gsfc.nasa.gov/14126/#media_group_314975", "widget": "Video player", "title": "", "caption": "", "description": "On August 31, 2012 a long filament of solar material that had been hovering in the sun's atmosphere, the corona, erupted out into space at 4:36 p.m. EDT. The coronal mass ejection, or CME, traveled at over 900 miles per second. The CME did not travel directly toward Earth, but did connect with Earth's magnetic environment, or magnetosphere, with a glancing blow. causing aurora to appear on the night of Monday, September 3.
4k source material", "items": [ { "id": 213403, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 372201, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/Magnificent_Eruption_Mk_II-overlay.00180_print.jpg", "filename": "Magnificent_Eruption_Mk_II-overlay.00180_print.jpg", "media_type": "Image", "alt_text": "On August 31, 2012 a long filament of solar material that had been hovering in the sun's atmosphere, the corona, erupted out into space at 4:36 p.m. EDT. The coronal mass ejection, or CME, traveled at over 900 miles per second. The CME did not travel directly toward Earth, but did connect with Earth's magnetic environment, or magnetosphere, with a glancing blow. causing aurora to appear on the night of Monday, September 3.4k source material", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 213401, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 372199, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/Magnificent_Eruption_Mk_II-overlay.mp4", "filename": "Magnificent_Eruption_Mk_II-overlay.mp4", "media_type": "Movie", "alt_text": "On August 31, 2012 a long filament of solar material that had been hovering in the sun's atmosphere, the corona, erupted out into space at 4:36 p.m. EDT. The coronal mass ejection, or CME, traveled at over 900 miles per second. The CME did not travel directly toward Earth, but did connect with Earth's magnetic environment, or magnetosphere, with a glancing blow. causing aurora to appear on the night of Monday, September 3.4k source material", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 213402, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 372200, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/Magnificent_Eruption_Mk_II-overlay.webm", "filename": "Magnificent_Eruption_Mk_II-overlay.webm", "media_type": "Movie", "alt_text": "On August 31, 2012 a long filament of solar material that had been hovering in the sun's atmosphere, the corona, erupted out into space at 4:36 p.m. EDT. The coronal mass ejection, or CME, traveled at over 900 miles per second. The CME did not travel directly toward Earth, but did connect with Earth's magnetic environment, or magnetosphere, with a glancing blow. causing aurora to appear on the night of Monday, September 3.4k source material", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 213400, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 372198, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/Magnificent_Eruption_Mk_II-overlay.mov", "filename": "Magnificent_Eruption_Mk_II-overlay.mov", "media_type": "Movie", "alt_text": "On August 31, 2012 a long filament of solar material that had been hovering in the sun's atmosphere, the corona, erupted out into space at 4:36 p.m. EDT. The coronal mass ejection, or CME, traveled at over 900 miles per second. The CME did not travel directly toward Earth, but did connect with Earth's magnetic environment, or magnetosphere, with a glancing blow. causing aurora to appear on the night of Monday, September 3.4k source material", "width": 1920, "height": 1080, "pixels": 2073600 } } ], "extra_data": {} }, { "id": 314976, "url": "https://svs.gsfc.nasa.gov/14126/#media_group_314976", "widget": "Video player", "title": "", "caption": "", "description": "On September 16, 2012 the sun had a beautiful prominence (see Wikipedia) that slowly twisted and dissipated over several hours. It was captured in 304 angstrom light by the Solar Dynamics Observatory's AIA instrument at 4k resolution and 12s imaging cadence. The prominence was immediately followed by one of the many eclipses that SDO experiences during September, when its orbit places the Earth between it and the sun.
4k source material", "items": [ { "id": 213407, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 372205, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/4033_Eclipse_mkII-1.00300_print.jpg", "filename": "4033_Eclipse_mkII-1.00300_print.jpg", "media_type": "Image", "alt_text": "On September 16, 2012 the sun had a beautiful prominence (see Wikipedia) that slowly twisted and dissipated over several hours. It was captured in 304 angstrom light by the Solar Dynamics Observatory's AIA instrument at 4k resolution and 12s imaging cadence. The prominence was immediately followed by one of the many eclipses that SDO experiences during September, when its orbit places the Earth between it and the sun.4k source material", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 213405, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 372203, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/4033_Eclipse_mkII-1.mp4", "filename": "4033_Eclipse_mkII-1.mp4", "media_type": "Movie", "alt_text": "On September 16, 2012 the sun had a beautiful prominence (see Wikipedia) that slowly twisted and dissipated over several hours. It was captured in 304 angstrom light by the Solar Dynamics Observatory's AIA instrument at 4k resolution and 12s imaging cadence. The prominence was immediately followed by one of the many eclipses that SDO experiences during September, when its orbit places the Earth between it and the sun.4k source material", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 213406, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 372204, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/4033_Eclipse_mkII-1.webm", "filename": "4033_Eclipse_mkII-1.webm", "media_type": "Movie", "alt_text": "On September 16, 2012 the sun had a beautiful prominence (see Wikipedia) that slowly twisted and dissipated over several hours. It was captured in 304 angstrom light by the Solar Dynamics Observatory's AIA instrument at 4k resolution and 12s imaging cadence. The prominence was immediately followed by one of the many eclipses that SDO experiences during September, when its orbit places the Earth between it and the sun.4k source material", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 213404, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 372202, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/4033_Eclipse_mkII-1.mov", "filename": "4033_Eclipse_mkII-1.mov", "media_type": "Movie", "alt_text": "On September 16, 2012 the sun had a beautiful prominence (see Wikipedia) that slowly twisted and dissipated over several hours. It was captured in 304 angstrom light by the Solar Dynamics Observatory's AIA instrument at 4k resolution and 12s imaging cadence. The prominence was immediately followed by one of the many eclipses that SDO experiences during September, when its orbit places the Earth between it and the sun.4k source material", "width": 1920, "height": 1080, "pixels": 2073600 } } ], "extra_data": {} }, { "id": 314977, "url": "https://svs.gsfc.nasa.gov/14126/#media_group_314977", "widget": "Video player", "title": "", "caption": "", "description": "The sun emitted an X1.8-class solar flare, peaking at 7:24 p.m. EST on Dec. 19, 2014. This image blends two wavelengths of extreme ultraviolet light, 171 (gold) and 131 (purple).
4k source material", "items": [ { "id": 213411, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 372209, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/Holiday_Lights_Blend_Move_MkIII.00150_print.jpg", "filename": "Holiday_Lights_Blend_Move_MkIII.00150_print.jpg", "media_type": "Image", "alt_text": "The sun emitted an X1.8-class solar flare, peaking at 7:24 p.m. EST on Dec. 19, 2014. This image blends two wavelengths of extreme ultraviolet light, 171 (gold) and 131 (purple).4k source material", "width": 1024, "height": 576, "pixels": 589824 } }, { "id": 213409, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 372207, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/Holiday_Lights_Blend_Move_MkIII.mp4", "filename": "Holiday_Lights_Blend_Move_MkIII.mp4", "media_type": "Movie", "alt_text": "The sun emitted an X1.8-class solar flare, peaking at 7:24 p.m. EST on Dec. 19, 2014. This image blends two wavelengths of extreme ultraviolet light, 171 (gold) and 131 (purple).4k source material", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 213410, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 372208, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/Holiday_Lights_Blend_Move_MkIII.webm", "filename": "Holiday_Lights_Blend_Move_MkIII.webm", "media_type": "Movie", "alt_text": "The sun emitted an X1.8-class solar flare, peaking at 7:24 p.m. EST on Dec. 19, 2014. This image blends two wavelengths of extreme ultraviolet light, 171 (gold) and 131 (purple).4k source material", "width": 1920, "height": 1080, "pixels": 2073600 } }, { "id": 213408, "type": "media", "extra_data": null, "title": null, "caption": null, "instance": { "id": 372206, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014126/Holiday_Lights_Blend_Move_MkIII.mov", "filename": "Holiday_Lights_Blend_Move_MkIII.mov", "media_type": "Movie", "alt_text": "The sun emitted an X1.8-class solar flare, peaking at 7:24 p.m. EST on Dec. 19, 2014. This image blends two wavelengths of extreme ultraviolet light, 171 (gold) and 131 (purple).4k source material", "width": 1920, "height": 1080, "pixels": 2073600 } } ], "extra_data": {} }, { "id": 314978, "url": "https://svs.gsfc.nasa.gov/14126/#media_group_314978", "widget": "Video player", "title": "", "caption": "", "description": "The sun emitted a mid-level solar flare, peaking at 3:01 p.m. EDT on Oct. 2, 2014.
This flare is classified as an M7.3 flare. M-class flares are one-tenth as powerful as the most powerful flares, which are designated X-class flares. This clip uses a blend of 304 and 171 angstrom light.
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Volunteers will use DSLR cameras on mounts that will track the Sun’s position in the sky to record changes in the Sun’s corona during the eclipse.Eclipse Megamovie is one of many participatory science projects happening during the 2024 total solar eclipse. Read more: https://science.nasa.gov/solar-system/skywatching/eclipse-photographers-help-study-sun-during-disappearing-act/ || ", "release_date": "2024-03-12T10:00:00-04:00", "update_date": "2024-04-25T13:33:20.145771-04:00", "main_image": { "id": 1089737, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014500/a014540/Thumbnail01.jpg", "filename": "Thumbnail01.jpg", "media_type": "Image", "alt_text": "Watch this video on the NASA Video YouTube channel.Complete transcript available.Music credit: \"Towards the Future\" by Evan William Conway [ASCAP] from Universal Production Music", "width": 1280, "height": 720, "pixels": 921600 } }, { "id": 14133, "url": "https://svs.gsfc.nasa.gov/14133/", "page_type": "Produced Video", "title": "Concert videos", "description": "These videos are designed to accompany live orchestral performances. For more information and inquiries about their use, please contact Scott Wiessinger at scott.wiessinger@nasa.gov. || ", "release_date": "2022-04-06T13:00:00-04:00", "update_date": "2023-08-15T16:23:32.431926-04:00", "main_image": { "id": 372077, "url": "https://svs.gsfc.nasa.gov/vis/a010000/a014100/a014133/Concert_SDO_HELIOS_FINAL_ProRes_1920x1080.05667_print.jpg", "filename": "Concert_SDO_HELIOS_FINAL_ProRes_1920x1080.05667_print.jpg", "media_type": "Image", "alt_text": "This video contains imagery of the Sun from the Solar Dynamics Observatory (SDO). Much of this footage is in ultraviolet light and shows the hot atmosphere of the Sun, called the corona. It is edited to accompany Carl Nielsen's Helios Overture.", "width": 1024, "height": 576, "pixels": 589824 } } ], "newer_versions": [], "older_versions": [], "alternate_versions": [] }