Image:Yohkohimage.gif

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source: http://ydac.mssl.ucl.ac.uk/ydac/

This image is a full-disk view of the X-ray Sun and was produced by the Yohkoh solar observatory in 1991. The structures that can be seen consist of large and hot (>2MK) coronal magnetic structures. This particular image, one of millions, shows a quite active corona from near the maximum of the solar cycle. At the upper right (solar northwest) one can see an "X-ray jet") squirting outwards - this was one of Yohkoh's original discoveries.


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current20:23, 29 January 2007512×512 (228 KB)Eeron80 (Talk | contribs) (source: http://ydac.mssl.ucl.ac.uk/ydac/ This image is a full-disk view of the X-ray Sun and was produced by the ''Yohkoh'' solar observatory in 1991. The structures that can be seen consist of large and hot (>2MK) coronal loop structures. )

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