Fig. 2


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Hinode/EIS produced a mosaic of slot images on 11 February 2010, to form a series of full disk images in spectral lines formed at temperatures ranging from <105 K (He ii) to ~3 × 106 K (Fe xvi), thereby illustrating the multithermal structuring of the EUV corona. (Photo credit: JAXA/NASA/ESA Hinode/EIS).

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