SDO HMI 2011-10-10 02:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.31 | 196.87 | 18.88 | 111.32 | 23.46 | 154.16 | 23.95 | 309.43 | 0.4841 | -455.0 | -348.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.94 | 182.32 | 5.07 | 103.36 | 23.08 | 155.02 | 24.81 | 307.75 | 0.4901 | -1014.9 | -437.0 | |
| 24.37 | -1.00 | 13.81 | -1.00 | 23.35 | 154.64 | 24.43 | 308.59 | 0.4878 | -1294.7 | 999999 | |
| 0.00 | 1.58 | 0.00 | 0.88 | 26.15 | 150.18 | 19.97 | 318.49 | 0.4644 | 604.0 | 514.1 | |
| 0.00 | 1.31 | 0.00 | 0.71 | 23.50 | 148.08 | 17.87 | 316.96 | 0.4141 | 763.0 | 651.0 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 25.99 | 148.32 | 18.11 | 320.82 | 0.4440 | 507.0 | 420.6 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 25.88 | 147.98 | 17.77 | 321.12 | 0.4393 | 865.0 | 715.9 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 25.18 | 147.88 | 17.66 | 320.15 | 0.4304 | 713.0 | 487.0 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 24.08 | 147.68 | 17.47 | 318.59 | 0.4161 | 720.0 | 606.3 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 25.66 | 147.71 | 17.49 | 321.19 | 0.4342 | 743.0 | 534.3 | |
| 0.00 | 1.58 | 0.00 | 0.87 | 26.34 | 147.43 | 17.21 | 322.68 | 0.4393 | 707.0 | 572.0 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 26.19 | 144.87 | 14.66 | 326.59 | 0.4141 | 868.0 | 801.4 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 26.03 | 144.78 | 14.57 | 326.51 | 0.4114 | 937.0 | 760.3 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 24.29 | 142.11 | 11.89 | 328.93 | 0.3656 | 810.0 | 610.4 | |
| 0.00 | 1.40 | 0.00 | 0.78 | 30.09 | 142.54 | 12.33 | 335.56 | 0.4483 | 737.0 | 507.3 | |
| 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. | |