SDO's Multi-wavelength View of a May 2013 Solar Flare

  • Released Tuesday, February 11, 2014
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An active region on the left limb of the Sun launches a large flare and coronal material in this sequence from early May 2013.

A view of the flare in the 13.1nm filter. The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise. The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD. The 'waffle' pattern is also an artifact of the imaging system with bright events.

4Kx4K full resolution images. A view of the flare in the 13.1nm filter. The flare mode alters the exposure of the camera which results in some flickering in the exposure-adjusted images due to the changing relative levels of the noise. The bright vertical line through the flare is due to excess charge in the pixels receiving the flare leaking out through the readout line in the CCD. The 'waffle' pattern is also an artifact of the imaging system with bright events.



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Please give credit for this item to:
NASA's Scientific Visualization Studio, the SDO Science Team, and the Virtual Solar Observatory.

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This page was originally published on Tuesday, February 11, 2014.
This page was last updated on Friday, August 2, 2024 at 3:24 PM EDT.


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