File:X5.4 solar flare seen by SDO in 131 Å extreme ultraviolet light.jpg

From Wikimedia Commons, the free media repository
Jump to navigation Jump to search

Original file ‎(4,096 × 4,096 pixels, file size: 5.93 MB, MIME type: image/jpeg)

Captions

Captions

Add a one-line explanation of what this file represents
Description

The powerful March 7, 2012 solar flare, which earned a classification of X5.4 based on the peak intensity of its X-rays, is the strongest eruption so far observed by Fermi's LAT. The flare produced such an outpouring of gamma rays — a form of light with even greater energy than X-rays — that the Sun briefly became the brightest object in the gamma-ray sky. See this NASA video for more information about X5.4 and the process behind solar flares producing gamma rays.

This is a full disk image of the flare in 131 angstrom extreme ultraviolet light.
Date
Source http://svs.gsfc.nasa.gov/goto?11000 (direct link)
Author NASA/Goddard Space Flight Center
Permission
(Reusing this file)
Public domain 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:
Other versions
X5.4 in 171 Å extreme ultraviolet light

File history

Click on a date/time to view the file as it appeared at that time.

Date/TimeThumbnailDimensionsUserComment
current16:10, 11 July 2012Thumbnail for version as of 16:10, 11 July 20124,096 × 4,096 (5.93 MB)Prof. Professorson (talk | contribs){{Information |Description=The powerful March 7, 2012 solar flare, which earned a classification of X5.4 based on the peak intensity of its X-rays, is the strongest eruption so far observed by Fermi's LAT. The flare p...

You cannot overwrite this file.

File usage on other wikis

The following other wikis use this file:

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.

Retrieved from "https://commons.wikimedia.org/w/index.php?title=File:X5.4_solar_flare_seen_by_SDO_in_131_Å_extreme_ultraviolet_light.jpg&oldid=794823927"