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This one could be called "Relationship between a CME-driven shock and a coronal metric type II burst", excerpted, from Y. Liu. But I prefer to call it 'sunset on the sea':

If you click on the image, you can see the full data plot, taken (without forewarning to the scientists) from their online powerpoint slides.
This one is either "STEREO small ICME activity" by K.E.J. Huttunen, or "butterflies".

Currently, I'm comparing two different models for an erupting CME, one an idealized fluxrope 'loop' and the other a direct reconstruction of the data. Neither evokes the real world such as the two above, n
or do they have sufficient information density to give the stronger pallet of the other datas. In short, they're ugly and jaggy. But it is fun to look at data in different ways. Which color is better?


Until next week,
Alex








I once stumbled upon a paper by M. Zingale et. al.: "Helium Detonations on Neutron Stars", when it was published back in 2001. In the paper the team presents some visualisations of their simulations. Those images are absolutely stunning. I always thought it was a pity that they were "only science results". Check them out at http://www.astro.sunysb.edu/mzingale/xray_gallery/.
Regards
- Frank