| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.95 | 151.71 | 42.15 | 176.42 | 7.70 | 129.54 | -64.69 | 82.06 | 0.9055 | -49.4 | -147.4 | |
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back to the solar disc SDO HMI 2011-11-28 20:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 1.21 | 9.17 | 131.32 | -62.90 | 80.33 | 0.8934 | 428.0 | 374.7 | |
| 12.65 | 83.42 | 13.72 | 90.30 | 7.56 | 131.46 | -62.77 | 82.13 | 0.8917 | -695.8 | -311.5 | |
| 0.00 | 1.03 | 0.00 | 1.14 | 7.91 | 130.83 | -63.39 | 81.77 | 0.8967 | 249.0 | 238.0 | |
| 0.00 | 0.60 | 0.00 | 0.66 | 5.73 | 130.82 | -63.40 | 84.20 | 0.8962 | -379.0 | -411.4 | |
| 0.00 | 2.39 | 0.00 | 2.71 | 7.21 | 130.27 | -63.95 | 82.57 | 0.9007 | -516.0 | -356.0 | |
| 2.05 | 2.39 | 2.31 | 2.70 | 6.41 | 130.33 | -63.89 | 83.47 | 0.9000 | -410.0 | -382.8 | |
| 0.00 | 2.31 | 0.00 | 2.58 | 5.49 | 130.53 | -63.69 | 84.48 | 0.8983 | -500.0 | -382.9 | |
| 0.00 | 2.05 | 0.00 | 2.32 | 6.67 | 130.20 | -64.02 | 83.18 | 0.9011 | -333.0 | -215.6 | |
| 0.00 | 0.85 | 0.00 | 0.98 | 7.26 | 129.84 | -64.38 | 82.53 | 0.9039 | -283.0 | -219.8 | |
| 2.56 | 9.92 | 3.02 | 11.74 | 7.64 | 129.10 | -65.12 | 82.15 | 0.9094 | -264.8 | 96.6 | |
| 2.05 | 3.33 | 2.42 | 3.93 | 6.95 | 129.08 | -65.14 | 82.91 | 0.9094 | -269.0 | -168.1 | |
| 0.00 | 0.94 | 0.00 | 1.16 | 8.24 | 128.03 | -66.19 | 81.53 | 0.9171 | -141.0 | -151.2 | |
| 0.00 | 2.31 | 0.00 | 2.83 | 7.98 | 128.12 | -66.10 | 81.82 | 0.9165 | 382.0 | 264.3 | |
| 3.76 | 7.52 | 4.71 | 9.40 | 8.74 | 127.64 | -66.59 | 81.00 | 0.9200 | 494.7 | 439.8 | |
| 7.52 | 31.54 | 10.01 | 42.76 | 8.27 | 126.16 | -68.07 | 81.58 | 0.9296 | 606.3 | 119.8 | |
| 4.36 | -15.00 | 5.96 | -15.00 | 7.90 | 125.47 | -68.75 | 82.01 | 0.9338 | 354.1 | 999999 | |
| 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. | |