SDO HMI 2011-10-12 22:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.17 | 110.89 | 22.61 | 56.79 | 20.07 | 97.35 | 4.52 | 342.84 | 0.2551 | -227.3 | -4.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.27 | 46.79 | 4.77 | 24.05 | 21.27 | 96.73 | 3.90 | 346.44 | 0.2713 | 993.8 | 840.0 | |
| 3.15 | -1.00 | 1.62 | -1.00 | 21.15 | 96.21 | 3.38 | 348.09 | 0.2674 | 1072.1 | 999999 | |
| 1.31 | -1.00 | 0.67 | -1.00 | 21.09 | 95.89 | 3.06 | 349.15 | 0.2654 | 879.2 | 999999 | |
| 1.31 | -1.00 | 0.67 | -1.00 | 21.05 | 96.92 | 4.08 | 345.61 | 0.2685 | 896.9 | 999999 | |
| 1.75 | -1.00 | 0.90 | -1.00 | 20.90 | 96.59 | 3.76 | 346.57 | 0.2647 | 1006.5 | 999999 | |
| 1.05 | -1.00 | 0.54 | -1.00 | 20.75 | 96.49 | 3.66 | 346.77 | 0.2618 | 906.3 | 999999 | |
| 0.00 | 2.10 | 0.00 | 1.08 | 20.63 | 95.91 | 3.08 | 348.70 | 0.2577 | 1087.0 | 800.4 | |
| 0.00 | 0.61 | 0.00 | 0.31 | 19.99 | 98.23 | 5.39 | 339.88 | 0.2580 | -513.0 | -509.1 | |
| 0.00 | 1.22 | 0.00 | 0.63 | 19.81 | 98.26 | 5.42 | 339.53 | 0.2552 | -815.0 | -677.3 | |
| 0.00 | 2.10 | 0.00 | 1.07 | 19.53 | 98.34 | 5.51 | 338.81 | 0.2514 | -758.0 | -636.4 | |
| 16.53 | 58.07 | 8.44 | 29.65 | 19.22 | 98.17 | 5.34 | 338.94 | 0.2456 | -1008.6 | -754.5 | |
| 3.50 | -11.00 | 1.79 | -11.00 | 19.23 | 97.47 | 4.64 | 341.50 | 0.2416 | -994.4 | 999999 | |
| 3.59 | -11.00 | 1.83 | -11.00 | 19.14 | 97.88 | 5.05 | 339.85 | 0.2424 | -1298.9 | 999999 | |
| 2.71 | -11.00 | 1.38 | -11.00 | 19.08 | 97.63 | 4.79 | 340.70 | 0.2400 | -1045.6 | 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. | |