This still from STEREO images shows data from the Jan. 24-25, 2007 coronal mass ejection. The spiky feature towards the lower left are caused by the remnants of Comet McNaught's tail. Credit: NASA/NRL. Click to enlarge.
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This still from STEREO images shows data from the Jan. 24-25, 2007 coronal mass ejection. The spiky feature towards the lower left are caused by the remnants of Comet McNaught's tail. Credit: NASA/NRL. Click to enlarge. |
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