SDO HMI 2011-10-25 06:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.82 | 209.75 | 26.70 | 156.57 | -21.71 | 331.34 | 41.18 | 234.84 | 0.7503 | -516.3 | -325.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.13 | 0.00 | 0.94 | -19.70 | 338.37 | 48.21 | 240.88 | 0.8057 | 527.0 | 405.7 | |
| 0.00 | 1.74 | 0.00 | 1.43 | -19.32 | 338.13 | 47.96 | 241.20 | 0.8020 | 552.0 | 354.9 | |
| 0.00 | 2.52 | 0.00 | 2.07 | -19.01 | 337.91 | 47.75 | 241.46 | 0.7989 | 583.0 | 470.0 | |
| 0.00 | 1.30 | 0.00 | 1.06 | -19.02 | 337.45 | 47.28 | 241.25 | 0.7945 | 490.0 | 396.0 | |
| 2.52 | 7.21 | 2.02 | 5.81 | -18.76 | 336.98 | 46.81 | 241.33 | 0.7891 | 697.1 | 610.7 | |
| 0.00 | 0.61 | 0.00 | 0.49 | -18.49 | 336.88 | 46.72 | 241.60 | 0.7871 | 685.0 | 619.3 | |
| 0.00 | 1.13 | 0.00 | 0.91 | -19.18 | 336.95 | 46.78 | 240.83 | 0.7906 | 589.0 | 473.7 | |
| 0.00 | 0.26 | 0.00 | 0.21 | -19.46 | 336.87 | 46.71 | 240.46 | 0.7911 | 462.0 | 476.0 | |
| 0.00 | 1.30 | 0.00 | 1.04 | -19.04 | 336.39 | 46.23 | 240.73 | 0.7848 | 717.0 | 545.4 | |
| 5.56 | 191.59 | 4.13 | 141.93 | -21.40 | 331.22 | 41.06 | 235.19 | 0.7472 | -780.3 | -409.5 | |
| 3.48 | -10.00 | 2.59 | -10.00 | -21.75 | 331.09 | 40.93 | 234.69 | 0.7480 | -629.5 | 999999 | |
| 0.96 | -10.00 | 0.71 | -10.00 | -22.05 | 331.11 | 40.95 | 234.35 | 0.7499 | -567.9 | 999999 | |
| 23.30 | -10.00 | 17.25 | -10.00 | -22.15 | 330.59 | 40.43 | 233.91 | 0.7456 | -1084.9 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.68 | -20.96 | 328.29 | 38.13 | 233.86 | 0.7163 | -472.0 | -404.5 | |
| 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. | |