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imported>Hhudson (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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Latest revision as of 14:35, 1 November 2024
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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| current | 14:35, 1 November 2024 |  | 982 × 802 (202 KB) | Maintenance script (talk | contribs) | == Summary == Importing file |
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