| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.89 | 45.17 | 25.12 | 44.23 | 19.39 | 87.39 | 58.75 | 290.78 | 0.8642 | -27.7 | -60.2 | |
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back to the solar disc SDO HMI 2011-11-14 02:58:58 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 | 1.15 | 15.98 | 92.13 | 63.49 | 286.35 | 0.8984 | 419.0 | 367.0 | |
| 0.00 | 0.95 | 0.00 | 1.16 | 21.82 | 94.23 | 65.59 | 292.55 | 0.9171 | 143.0 | 126.9 | |
| 7.05 | 13.08 | 7.15 | 13.27 | 19.33 | 88.62 | 59.98 | 290.51 | 0.8744 | -423.2 | -280.7 | |
| 3.70 | 4.82 | 3.68 | 4.79 | 19.32 | 87.93 | 59.29 | 290.61 | 0.8689 | -554.9 | -457.1 | |
| 0.00 | 1.03 | 0.00 | 1.00 | 19.33 | 87.13 | 58.49 | 290.74 | 0.8623 | -345.0 | -323.8 | |
| 8.69 | 11.36 | 8.14 | 10.64 | 18.41 | 85.92 | 57.28 | 289.87 | 0.8509 | 581.2 | 352.2 | |
| 0.00 | 1.12 | 0.00 | 1.07 | 19.75 | 86.66 | 58.02 | 291.31 | 0.8589 | 322.0 | 201.5 | |
| 1.20 | 1.63 | 1.16 | 1.57 | 20.01 | 86.62 | 57.98 | 291.61 | 0.8590 | 257.6 | 95.0 | |
| 0.86 | 1.38 | 0.80 | 1.27 | 18.56 | 85.41 | 56.78 | 290.13 | 0.8467 | 480.3 | 294.0 | |
| 0.00 | 0.77 | 0.00 | 0.73 | 19.78 | 86.02 | 57.38 | 291.45 | 0.8536 | 247.0 | 268.6 | |
| 1.12 | 2.24 | 1.08 | 2.15 | 21.30 | 86.51 | 57.87 | 293.12 | 0.8599 | -336.1 | -370.8 | |
| 3.27 | 4.30 | 3.11 | 4.09 | 21.32 | 86.04 | 57.40 | 293.23 | 0.8561 | -630.9 | -568.1 | |
| 0.00 | 1.46 | 0.00 | 1.34 | 19.46 | 84.85 | 56.22 | 291.27 | 0.8431 | 332.0 | 231.9 | |
| 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. | |