File:NASA – Thermonuclear Art – The Sun In Ultra-HD (4K).webm
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Size of this JPG preview of this WEBM file: 800 × 450 pixels. Other resolutions: 320 × 180 pixels | 640 × 360 pixels | 1,024 × 576 pixels | 1,280 × 720 pixels | 2,560 × 1,440 pixels | 3,840 × 2,160 pixels.
Original file (WebM audio/video file, VP9/Opus, length 30 min 24 s, 3,840 × 2,160 pixels, 18.47 Mbps overall, file size: 3.92 GB)
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| Description |
English: The Sun is always changing and NASA's Solar Dynamics Observatory is always watching. Launched on February 11, 2010, SDO keeps a 24-hour eye on teh entire disk of The Sun, with a prime view of hte graceful dance of solar material coursing through The Sun's atmosphere, the corona. |
| Date | |
| Source | http://svs.gsfc.nasa.gov/12034 |
| Author | NASA, The SDO Team, Genna Duberstein and Scott Wiessinger, Producers |
| Other versions | 1080p |
Licensing[edit]
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This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) |  |
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This file was selected as the media of the day for 02 August 2017. It was captioned as follows:
English: It’s always shining, always ablaze with light and energy that drive weather, biology and more. In addition to keeping life alive on Earth, the sun also sends out a constant flow of particles called the solar wind, and it occasionally erupts with giant clouds of solar material, called coronal mass ejections, or explosions of X-rays called solar flares.
Other languages
Čeština: Video s vysokým rozlišením natočené sondou Solar Dynamics Observatory, zachycující jevy na povrchu Slunce jako protuberance, výron koronální hmoty, vznik slunečního větru nebo sluneční erupce. English: It’s always shining, always ablaze with light and energy that drive weather, biology and more. In addition to keeping life alive on Earth, the sun also sends out a constant flow of particles called the solar wind, and it occasionally erupts with giant clouds of solar material, called coronal mass ejections, or explosions of X-rays called solar flares. Polski: Zawsze świeci, zawsze promieniuje światłem i energią, która wpływa na pogodę, biologię i inne rzeczy. Oprócz utrzymywania życia na Ziemi, Słońce emituje także stały strumień cząstek nazywany wiatrem słonecznym, a czasami wybucha tworząc olbrzymie chmury materii słonecznej, co jest nazywane koronalnymi wyrzutami masy, lub eksploduje emitując promieniowanie rentgenowskie, co z kolei jest nazywane rozbłyskami słonecznymi.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 03:28, 22 July 2017 | 30 min 24 s, 3,840 × 2,160 (3.92 GB) | Brooke Vibber (talk | contribs) |
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File usage on Commons
The following 21 pages use this file:
- User:Atlasowa/New video2commons/2017 July 21-31
- Commons:WikiProject Aviation/recent uploads/2017 July 22
- File:Knowledge belongs to all of us - 2030.wikimedia.org.webm
- File:NASA - Thermonuclear Art – The Sun In Ultra-HD (4K).webm (file redirect)
- Template:Potd/2017-08
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- User:Atlasowa/New video2commons/2017 July 21-31
- Commons:WikiProject Aviation/recent uploads/2017 July 22
- Template:Motd/2017-08-02
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- Template:Motd/2017-08-02 (mk)
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- File:Knowledge belongs to all of us - 2030.wikimedia.org.webm
- Template:Motd/2017-08
- Template:Motd/2017-08-02
- Template:Motd/2017-08-02 (cs)
- Template:Motd/2017-08-02 (en)
- Template:Motd/2017-08-02 (mk)
- Template:Motd/2017-08-02 (pl)
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