SDO HMI 2011-12-07 11:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.57 | 23.44 | 4.54 | 17.49 | 18.68 | 125.73 | 45.15 | 295.80 | 0.7436 | 379.3 | 133.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 0.91 | 16.94 | 138.42 | 57.84 | 289.73 | 0.8624 | -365.0 | -334.5 | |
| 0.00 | 1.28 | 0.00 | 1.19 | 16.72 | 136.83 | 56.25 | 289.81 | 0.8485 | 361.0 | 292.3 | |
| 0.00 | 1.02 | 0.00 | 0.95 | 17.03 | 136.86 | 56.28 | 290.16 | 0.8493 | 155.0 | 147.7 | |
| 0.00 | 0.85 | 0.00 | 0.79 | 16.88 | 136.57 | 55.99 | 290.04 | 0.8465 | 471.0 | 390.5 | |
| 0.00 | 2.13 | 0.00 | 1.59 | 18.37 | 126.28 | 45.70 | 294.81 | 0.7506 | -612.0 | -524.0 | |
| 0.00 | 1.62 | 0.00 | 1.24 | 20.44 | 126.77 | 46.19 | 297.24 | 0.7628 | -679.0 | -543.2 | |
| 6.57 | 8.19 | 4.54 | 5.66 | 18.31 | 121.70 | 41.12 | 296.61 | 0.7007 | 805.3 | 534.8 | |
| 0.00 | 2.30 | 0.00 | 1.59 | 18.72 | 121.57 | 40.99 | 297.22 | 0.7010 | 443.0 | 338.5 | |
| 0.00 | 0.60 | 0.00 | 0.43 | 22.12 | 122.62 | 42.04 | 301.18 | 0.7274 | 608.0 | 510.4 | |
| 0.00 | 1.36 | 0.00 | 0.95 | 20.09 | 121.25 | 40.67 | 299.22 | 0.7036 | 604.0 | 417.1 | |
| 0.00 | 1.53 | 0.00 | 1.07 | 20.82 | 121.02 | 40.44 | 300.29 | 0.7045 | 451.0 | 410.9 | |
| 0.00 | 1.11 | 0.00 | 0.77 | 20.82 | 120.77 | 40.19 | 300.42 | 0.7018 | 522.0 | 465.7 | |
| 0.00 | 0.51 | 0.00 | 0.35 | 20.28 | 119.74 | 39.16 | 300.24 | 0.6880 | 659.0 | 550.0 | |
| 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. | |