| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.46 | 275.33 | 25.64 | 142.64 | 17.70 | 223.36 | 4.99 | 343.53 | 0.2935 | -744.8 | -351.3 | |
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back to the solar disc SDO HMI 2011-11-27 00:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.03 | 0.00 | 0.54 | 19.69 | 224.87 | 6.49 | 341.22 | 0.3323 | -604.0 | -481.1 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 18.11 | 224.28 | 5.90 | 341.19 | 0.3045 | -394.0 | -226.5 | |
| 13.86 | 235.30 | 7.17 | 121.90 | 17.40 | 224.00 | 5.63 | 341.21 | 0.2918 | -1258.2 | -409.7 | |
| 0.26 | -3.00 | 0.13 | -3.00 | 17.13 | 223.84 | 5.46 | 341.40 | 0.2866 | -1108.0 | 999999 | |
| 30.12 | -3.00 | 15.61 | -3.00 | 17.81 | 223.39 | 5.02 | 343.54 | 0.2951 | -1273.5 | 999999 | |
| 2.74 | 3.59 | 1.44 | 1.89 | 20.13 | 223.27 | 4.90 | 345.96 | 0.3318 | 867.7 | 720.2 | |
| 0.00 | 1.88 | 0.00 | 0.99 | 19.95 | 222.57 | 4.20 | 347.77 | 0.3262 | -712.0 | -528.7 | |
| 0.00 | 5.13 | 0.00 | 2.62 | 15.08 | 222.12 | 3.75 | 345.01 | 0.2452 | 819.0 | 786.2 | |
| 2.48 | 12.06 | 1.29 | 6.25 | 18.30 | 221.97 | 3.59 | 348.40 | 0.2974 | -819.4 | -887.6 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 19.82 | 221.81 | 3.44 | 349.85 | 0.3218 | -624.0 | -468.9 | |
| 0.00 | 1.97 | 0.00 | 1.01 | 15.69 | 221.74 | 3.36 | 347.09 | 0.2537 | 754.0 | 646.3 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 15.14 | 221.67 | 3.29 | 346.84 | 0.2443 | 998.0 | 818.6 | |
| 0.00 | 1.80 | 0.00 | 0.92 | 15.42 | 221.52 | 3.14 | 347.66 | 0.2483 | 983.0 | 838.0 | |
| 0.00 | 1.71 | 0.00 | 0.89 | 19.33 | 221.46 | 3.08 | 350.62 | 0.3126 | -859.0 | -645.6 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 19.67 | 221.40 | 3.03 | 350.97 | 0.3181 | -766.0 | -635.2 | |
| 0.00 | 3.76 | 0.00 | 1.95 | 18.40 | 220.63 | 2.25 | 352.70 | 0.2953 | 749.0 | 672.0 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 18.52 | 219.82 | 1.44 | 355.35 | 0.2959 | 837.0 | 636.2 | |
| 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. | |