SDO HMI 2011-08-07 05:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.19 | 56.96 | 7.36 | 29.57 | 18.98 | 241.87 | -11.93 | 40.95 | 0.2987 | 154.7 | 303.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.65 | 18.06 | 246.77 | -7.03 | 29.40 | 0.2381 | -915.0 | -765.1 | |
| 0.00 | 6.78 | 0.00 | 3.49 | 18.64 | 244.02 | -9.78 | 36.55 | 0.2715 | -1124.0 | -941.3 | |
| 4.97 | 7.05 | 2.56 | 3.63 | 18.29 | 243.68 | -10.12 | 38.29 | 0.2704 | -988.8 | -706.0 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 18.91 | 243.61 | -10.19 | 37.02 | 0.2791 | -783.0 | -571.2 | |
| 2.35 | 4.07 | 1.22 | 2.11 | 19.58 | 242.32 | -11.48 | 38.75 | 0.3008 | -798.4 | -612.1 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 18.97 | 241.74 | -12.06 | 41.48 | 0.2996 | 954.0 | 796.2 | |
| 0.00 | 3.07 | 0.00 | 1.59 | 18.37 | 241.45 | -12.34 | 43.55 | 0.2957 | 1055.0 | 791.6 | |
| 0.00 | 2.17 | 0.00 | 1.13 | 19.74 | 241.02 | -12.78 | 41.33 | 0.3166 | 802.0 | 591.3 | |
| 4.25 | 18.26 | 2.21 | 9.50 | 18.80 | 241.06 | -12.74 | 43.38 | 0.3052 | 1179.7 | 872.0 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 18.82 | 240.66 | -13.13 | 44.18 | 0.3100 | 751.0 | 666.9 | |
| 2.62 | 8.77 | 1.37 | 4.59 | 19.72 | 240.46 | -13.34 | 42.53 | 0.3227 | 837.7 | 743.1 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 19.28 | 240.33 | -13.47 | 43.79 | 0.3191 | 791.0 | 633.9 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 21.10 | 238.99 | -14.81 | 42.45 | 0.3548 | 751.0 | 572.2 | |
| 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. | |