File:August 2010 CME SDO.jpg
Summary
One of the four <a href="https://en.wikipedia.org/wiki/coronal_mass_ejection" class="extiw" title="en:coronal mass ejection">coronal mass ejections</a> on 1 August 2010, as seen in <a href="https://en.wikipedia.org/wiki/extreme_ultraviolet" class="extiw" title="en:extreme ultraviolet">extreme ultraviolet</a> light by the <a href="https://en.wikipedia.org/wiki/Solar_Dynamics_Observatory" class="extiw" title="en:Solar Dynamics Observatory">Solar Dynamics Observatory</a>.
Original caption: "On August 1st, almost the entire Earth-facing side of the sun erupted in a tumult of activity. There was a C3-class solar flare, a solar tsunami, multiple filaments of magnetism lifting off the stellar surface, large-scale shaking of the solar corona, radio bursts, a coronal mass ejection and more. This extreme ultraviolet snapshot from the Solar Dynamics Observatory shows the sun's northern hemisphere in mid-eruption. Different colors in the image represent different gas temperatures ranging from ~1 to 2 million degrees K. Credit: NASA/SDO"
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 01:39, 17 January 2017 | | 1,279 × 718 (120 KB) | 127.0.0.1 (talk) | One of the four <a href="https://en.wikipedia.org/wiki/coronal_mass_ejection" class="extiw" title="en:coronal mass ejection">coronal mass ejections</a> on 1 August 2010, as seen in <a href="https://en.wikipedia.org/wiki/extreme_ultraviolet" class="extiw" title="en:extreme ultraviolet">extreme ultraviolet</a> light by the <a href="https://en.wikipedia.org/wiki/Solar_Dynamics_Observatory" class="extiw" title="en:Solar Dynamics Observatory">Solar Dynamics Observatory</a>.<br>Original caption: "On August 1st, almost the entire Earth-facing side of the sun erupted in a tumult of activity. There was a C3-class solar flare, a solar tsunami, multiple filaments of magnetism lifting off the stellar surface, large-scale shaking of the solar corona, radio bursts, a coronal mass ejection and more. This extreme ultraviolet snapshot from the Solar Dynamics Observatory shows the sun's northern hemisphere in mid-eruption. Different colors in the image represent different gas temperatures ranging from ~1 to 2 million degrees K. Credit: NASA/SDO" |
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