File:210f2.png
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The line spectrum of the intensity (top left panel), the total linear polarization degree (top right), and the fractional Stokes parameters Q/I (bottom left), and U/I (bottom right), quantifying the direction and polarization in a non-magnetized model of the chromosphere. The radiation emission is strongest in the flare ribbon (from X=-3 Mm to X=3 Mm on the vertical axis) but the polarization is strongest at the edges of the ribbon.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 09:24, 21 October 2013 | | 982×802 (202 KB) | Hhudson (Talk | contribs) | (The line spectrum of the intensity (top left panel), the total linear polarization degree (top right), and the fractional Stokes parameters Q/I (bottom left), and U/I (bottom right), quantifying the direction and polarization in a non-magnetized model of ) |
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