SDO HMI 2011-11-29 14:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.78 | 84.09 | 16.61 | 56.22 | 18.05 | 223.72 | 39.36 | 296.12 | 0.6740 | -425.8 | -247.0 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 0.65 | 15.60 | 226.75 | 42.39 | 291.44 | 0.7000 | 436.0 | 302.5 | |
| 0.00 | 0.77 | 0.00 | 0.53 | 15.60 | 226.33 | 41.98 | 291.59 | 0.6951 | 507.0 | 508.8 | |
| 0.00 | 0.94 | 0.00 | 0.64 | 15.05 | 226.12 | 41.76 | 290.90 | 0.6908 | 716.0 | 614.5 | |
| 0.00 | 1.45 | 0.00 | 0.96 | 14.13 | 224.25 | 39.89 | 290.26 | 0.6653 | 648.0 | 552.4 | |
| 7.18 | 14.01 | 4.85 | 9.48 | 17.96 | 224.57 | 40.21 | 295.59 | 0.6834 | -700.4 | -482.1 | |
| 0.00 | 1.03 | 0.00 | 0.70 | 19.70 | 224.87 | 40.52 | 297.84 | 0.6941 | -639.0 | -506.9 | |
| 0.00 | 3.16 | 0.00 | 2.11 | 17.57 | 223.86 | 39.50 | 295.36 | 0.6734 | -726.0 | -612.5 | |
| 0.00 | 1.54 | 0.00 | 1.01 | 14.90 | 223.22 | 38.86 | 291.80 | 0.6554 | 665.0 | 569.1 | |
| 0.00 | 4.96 | 0.00 | 3.32 | 17.88 | 223.86 | 39.50 | 295.80 | 0.6747 | -743.0 | -686.7 | |
| 0.00 | 1.45 | 0.00 | 0.97 | 17.82 | 223.56 | 39.20 | 295.85 | 0.6710 | -784.0 | -550.1 | |
| 17.60 | 49.05 | 11.76 | 32.77 | 18.28 | 223.61 | 39.25 | 296.48 | 0.6735 | -900.3 | -302.1 | |
| 0.00 | 1.97 | 0.00 | 1.29 | 19.89 | 221.89 | 37.53 | 299.62 | 0.6613 | 490.0 | 329.3 | |
| 0.00 | 1.62 | 0.00 | 1.04 | 19.19 | 220.13 | 35.78 | 299.61 | 0.6373 | 579.0 | 502.9 | |
| 0.00 | 1.20 | 0.00 | 0.75 | 20.69 | 217.41 | 33.05 | 303.52 | 0.6143 | 654.0 | 456.1 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |