SDO HMI 2011-10-12 19:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.92 | 105.90 | 20.92 | 54.11 | 20.02 | 97.28 | 2.79 | 349.09 | 0.2470 | 29.4 | -191.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.66 | 31.13 | 4.44 | 15.98 | 21.21 | 96.33 | 1.84 | 353.47 | 0.2642 | 984.0 | 787.1 | |
| 1.66 | 8.66 | 0.85 | 4.44 | 21.07 | 95.97 | 1.48 | 354.68 | 0.2612 | 937.2 | 942.4 | |
| 5.95 | -1.00 | 3.05 | -1.00 | 21.26 | 96.72 | 2.23 | 352.12 | 0.2659 | 1008.1 | 999999 | |
| 1.05 | -2.00 | 0.54 | -2.00 | 20.90 | 96.14 | 1.65 | 353.99 | 0.2587 | 1176.0 | 999999 | |
| 2.71 | -1.00 | 1.39 | -1.00 | 21.06 | 96.88 | 2.39 | 351.46 | 0.2628 | 1069.5 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 20.85 | 96.68 | 2.19 | 352.02 | 0.2589 | 1025.0 | 749.1 | |
| 0.00 | 0.87 | 0.00 | 0.45 | 20.50 | 95.97 | 1.48 | 354.47 | 0.2516 | 831.0 | 660.6 | |
| 0.00 | 0.79 | 0.00 | 0.40 | 20.62 | 96.68 | 2.19 | 351.91 | 0.2549 | 872.0 | 772.2 | |
| 0.00 | 1.75 | 0.00 | 0.89 | 19.75 | 97.17 | 2.68 | 349.45 | 0.2418 | -761.0 | -375.8 | |
| 1.75 | 61.65 | 0.89 | 31.41 | 19.62 | 97.95 | 3.46 | 346.39 | 0.2424 | -919.0 | -746.4 | |
| 2.27 | -10.00 | 1.16 | -10.00 | 19.46 | 97.77 | 3.28 | 346.88 | 0.2390 | -942.8 | 999999 | |
| 2.10 | -10.00 | 1.07 | -10.00 | 19.25 | 97.41 | 2.92 | 348.09 | 0.2342 | -1045.0 | 999999 | |
| 5.68 | -10.00 | 2.89 | -10.00 | 19.11 | 97.64 | 3.15 | 347.05 | 0.2327 | -1250.7 | 999999 | |
| 9.09 | -10.00 | 4.64 | -10.00 | 19.22 | 98.11 | 3.62 | 345.35 | 0.2365 | -1067.0 | 999999 | |
| 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. | |