File:Illuminated line volume1.jpg
Original file (1,018 × 1,020 pixels, file size: 1.69 MB, MIME type: image/jpeg)
Summary[edit | edit source]
Description |
The stream lines on this computer simulation of a supernova show the flow of matter behind the shock wave giving clues as to the origin of pulsars. |
---|---|
Source |
The image appears on a website entitled, "Computer Science and Mathematics Division" at https://www.csm.ornl.gov/newsite/group_astro.html. |
Date |
2007 |
Author |
John Blondin and Anthony Mezzacappa |
Rationale |
No free licensed or public domain alternatives known to exist to show the stream lines by computer simulation of a supernova of the flow of matter behind the shock wave giving clues as to the origin of pulsars. |
Permission |
Fair Use, this file was deleted from commons on 8 August 2020 by c:user:JuTa for "there is no confidence that [Template:PD-OakRidge] is sufficient to ensure that this template can be used in a generic way for photographs published by Oak Ridge National Laboratory." |
This work is copyrighted. The individual who uploaded this work and first used it in an article, as well as subsequent persons who place it into articles, asserts that this qualifies as fair use of the material under United States copyright law.
This template must be accompanied by a {{Non-free media rationale}} justifying the assertion of fair use.
Note: The kinds of things that are considered acceptable for fair use on Wikiversity is significantly less than what is legally permitted. Please consult the Wikimedia Foundation Fair Use Policy to see if this content is permitted on Wikiversity under these further restrictions. Familiarize yourself with the Wikiversity Exemption Doctrine Policy before using this template.
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 21:55, 17 May 2021 | 1,018 × 1,020 (1.69 MB) | Marshallsumter (discuss | contribs) | {{Information1 |Description = The stream lines on this computer simulation of a supernova show the flow of matter behind the shock wave giving clues as to the origin of pulsars. |Source = The image appears on a website entitled, "Computer Science and Mathematics Division" at https://www.csm.ornl.gov/newsite/group_astro.html. |Date = 2007 |Author = John Blondin and Anthony Mezzacappa |Rationale = No free licensed or public domain alternatives known to exist to show the stream lines by computer... |
You cannot overwrite this file.
File usage
The following 4 pages use this file: