SDO HMI 2011-08-10 13:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.62 | 0.00 | 13.33 | 18.90 | 222.12 | 12.39 | 317.61 | 0.3025 | 72.5 | 110.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.26 | 0.00 | 0.67 | 20.41 | 226.70 | 16.97 | 312.10 | 0.3702 | -678.0 | -516.1 | |
| 0.00 | 4.33 | 0.00 | 2.29 | 20.01 | 225.41 | 15.68 | 313.36 | 0.3507 | -957.0 | -675.1 | |
| 0.00 | 2.17 | 0.00 | 1.13 | 17.95 | 224.29 | 14.55 | 310.51 | 0.3157 | -1002.0 | -784.9 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 18.65 | 223.75 | 14.02 | 313.25 | 0.3164 | -764.0 | -627.7 | |
| 0.00 | 1.26 | 0.00 | 0.66 | 18.50 | 223.70 | 13.97 | 312.96 | 0.3142 | -992.0 | -762.4 | |
| 0.00 | 1.72 | 0.00 | 0.89 | 19.45 | 221.87 | 12.13 | 319.07 | 0.3039 | 850.0 | 591.0 | |
| 0.00 | 1.99 | 0.00 | 1.03 | 19.14 | 221.51 | 11.78 | 319.18 | 0.2963 | 873.0 | 734.5 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 18.83 | 221.49 | 11.76 | 318.49 | 0.2923 | 691.0 | 550.8 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 14.21 | 220.83 | 11.09 | 306.58 | 0.2333 | -805.0 | -578.1 | |
| 0.00 | 3.97 | 0.00 | 2.05 | 18.19 | 220.83 | 11.09 | 318.53 | 0.2773 | 956.0 | 811.6 | |
| 0.00 | 2.89 | 0.00 | 1.49 | 18.23 | 220.37 | 10.64 | 319.78 | 0.2728 | 1127.0 | 901.4 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 19.11 | 218.15 | 8.41 | 328.05 | 0.2624 | 840.0 | 625.8 | |
| 0.00 | 1.53 | 0.00 | 0.79 | 21.91 | 215.30 | 5.57 | 341.46 | 0.2843 | 804.0 | 605.2 | |
| 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. | |