File:SDO 20100630 1024 0304 (AIA).ogv

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DescriptionSDO 20100630 1024 0304 (AIA).ogv	English: AIA 0304 channel is especially good at showing areas where cooler dense plumes of plasma (filaments and prominences) are located above the visible surface of the Sun. Many of these features either can't be seen or appear as dark lines in the other channels. The bright areas show places where the plasma has a high density. Where: Upper chromosphere and lower transition region Wavelength: 304 angstroms (0.0000000304 m) = Extreme Ultraviolet Primary ions seen: singly ionized helium (He II) Characteristic temperature: 50,000 K (90,000 F)
Date	Taken on 30 June 2010
Source	20100630_1024_0304
Author	Courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.

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Solar Dynamics Observatory
Credit and attribution belongs to the Atmospheric Imaging Assembly (AIA) team, NASA/GSFC/Solar Dynamics Observatory

This image or video was catalogued by Goddard Space Flight Center of the United States National Aeronautics and Space Administration (NASA) under Photo ID: 20100630_1024_0304.

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Format	Bitrate	Status	Encode time
VP9 720P	1.62 Mbps	Completed 00:03, 6 May 2024	12 s
VP9 480P	807 kbps	Completed 07:32, 6 May 2024	6.0 s
VP9 360P	461 kbps	Completed 07:31, 6 May 2024	5.0 s
VP9 240P	200 kbps	Completed 07:31, 6 May 2024	3.0 s
WebM 360P	577 kbps	Completed 07:31, 6 May 2024	1.0 s
QuickTime 144p (MJPEG)	1.02 Mbps	Completed 02:18, 26 November 2024	1.0 s

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