SDO HMI 2011-10-29 15:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.51 | 39.69 | 8.02 | 20.46 | 14.97 | 244.67 | 12.19 | 312.35 | 0.2773 | -160.4 | -56.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.70 | 19.93 | 6.07 | 10.33 | 14.39 | 246.95 | 14.47 | 305.32 | 0.2980 | -1123.6 | -663.0 | |
| 0.00 | 1.99 | 0.00 | 1.04 | 15.54 | 246.62 | 14.14 | 309.11 | 0.3046 | -839.0 | -647.7 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 15.01 | 244.34 | 11.85 | 312.43 | 0.2701 | -896.0 | -741.6 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 12.96 | 244.14 | 11.65 | 306.58 | 0.2463 | 901.0 | 688.9 | |
| 3.81 | 4.68 | 1.95 | 2.40 | 14.35 | 243.92 | 11.44 | 311.49 | 0.2577 | -1095.0 | -950.9 | |
| 0.00 | 1.30 | 0.00 | 0.67 | 16.98 | 242.18 | 9.69 | 323.12 | 0.2695 | 853.0 | 539.5 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 16.78 | 241.50 | 9.02 | 324.57 | 0.2601 | 768.0 | 476.6 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 14.91 | 240.42 | 7.94 | 323.25 | 0.2242 | 756.0 | 606.7 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 16.49 | 240.02 | 7.53 | 328.58 | 0.2423 | 953.0 | 700.4 | |
| 0.00 | 1.56 | 0.00 | 0.80 | 17.13 | 239.85 | 7.37 | 330.50 | 0.2501 | 806.0 | 563.8 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 16.34 | 239.64 | 7.15 | 329.55 | 0.2368 | 1032.0 | 861.8 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 16.68 | 239.46 | 6.98 | 330.88 | 0.2402 | 821.0 | 654.9 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 16.41 | 239.45 | 6.97 | 330.33 | 0.2361 | 750.0 | 592.8 | |
| 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. | |