File:183f2.png

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Distribution of flare radial locations at the extreme limb, now converted to units of solar radii. The vertical dotted line shows the theoretical height of the X-ray limb, as determined via model atmospheres and the cross-section for Compton scattering.

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current17:28, 27 August 2012Thumbnail for version as of 17:28, 27 August 2012340×340 (10 KB)Hhudson (Talk | contribs) (Distribution of flare radial locations at the extreme limb, now converted to units of solar radii. The vertical dotted line shows the theoretical height of the X-ray limb, as determined via model atmospheres and the cross-section for Compton scattering.)

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