File:Incandescent Sun.ogv
From Wikimedia Commons, the free media repository
Jump to navigation
Jump to search
Size of this JPG preview of this OGG file: 800 × 450 pixels. Other resolutions: 320 × 180 pixels | 640 × 360 pixels | 1,280 × 720 pixels.
Original file (Ogg multiplexed audio/video file, Theora/Vorbis, length 2 min 45 s, 1,280 × 720 pixels, 4.29 Mbps overall, file size: 84.56 MB)
File information
Structured data
Captions
Summary
[edit]DescriptionIncandescent Sun.ogv |
English: This video takes SDO images and applies additional processing to enhance the structures visible. While there is no scientific value to this processing, it does result in a beautiful, new way of looking at the sun. The original frames are in the 171 Angstrom wavelength of extreme ultraviolet. This wavelength shows plasma in the solar atmosphere, called the corona, that is around 600,000 Kelvin. The loops represent plasma held in place by magnetic fields. They are concentrated in "active regions" where the magnetic fields are the strongest. These active regions usually appear in visible light as sunspots. The events in this video represent 24 hours of activity on September 25, 2011. |
Date | |
Source | Goddard Multimedia |
Author | NASA/Goddard Space Flight Center |
This file was selected as the media of the day for 06 June 2012. It was captioned as follows:
English: This video takes SDO images of the sun and applies additional processing to enhance the structures visible. The events in this video represent 24 hours of activity on September 25, 2011.
Other languages
English: This video takes SDO images of the sun and applies additional processing to enhance the structures visible. The events in this video represent 24 hours of activity on September 25, 2011. Македонски: Снимка од Опсерваторијата за сончева динамика (SDO) со допонителна обработка за да се добие видливост на елементите. На снимката е прикажана активност во текот на 24 часа (25 септември 2011). 中文(简体):太阳动力学天文台拍摄到的太阳图像。图片已经过后期处理以显示结构细节。图片显示了2011年9月25日太阳一天的活动。
|
Licensing
[edit]Public domainPublic domainfalsefalse |
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.) | ||
Warnings:
|
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 09:15, 30 May 2012 | 2 min 45 s, 1,280 × 720 (84.56 MB) | Originalwana (talk | contribs) | {{Information |Description ={{en|1=This video takes SDO images and applies additional processing to enhance the structures visible. While there is no scientific value to this processing, it does result in a beautiful, new way of looking at the sun. ... |
You cannot overwrite this file.
File usage on Commons
The following 7 pages use this file:
Transcode status
Update transcode statusFile usage on other wikis
The following other wikis use this file:
- Usage on fa.wikipedia.org
- Usage on hi.wikipedia.org
- Usage on hi.wikiversity.org
- Usage on id.wikipedia.org
- Usage on ka.wikipedia.org
- Usage on pl.wikipedia.org
- Usage on pt.wikipedia.org
- Usage on te.wikipedia.org
- Usage on uk.wikipedia.org
- Usage on xmf.wikipedia.org
Metadata
This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
Software used |
---|