File:210f3.png
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After inclusion of a the effect of the vertical magnetic field with the intensity of 500 gauss, the polarization becomes practically radial with respect to the nearest solar limb (as quantified by the Q/I value while U/I is negligible).
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 10:34, 21 October 2013 | | 818×305 (74 KB) | Hhudson (Talk | contribs) | (After inclusion of a the effect of the vertical magnetic field with the intensity of 500 gauss, the polarization becomes practically radial with respect to the nearest solar limb (as quantified by the Q/I value while U/I is negligible).) |
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