SDO HMI 2011-08-10 06:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.50 | 0.00 | 9.55 | 19.20 | 223.63 | 10.05 | 324.01 | 0.2799 | -231.5 | -139.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.61 | 20.02 | 226.66 | 13.08 | 318.32 | 0.3211 | -1023.0 | -673.4 | |
| 0.00 | 2.26 | 0.00 | 1.18 | 20.29 | 226.12 | 12.53 | 320.05 | 0.3184 | -743.0 | -641.8 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 19.60 | 225.99 | 12.41 | 318.80 | 0.3088 | -853.0 | -653.2 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 19.74 | 225.48 | 11.89 | 320.27 | 0.3049 | -620.0 | -585.4 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 19.99 | 225.36 | 11.78 | 321.09 | 0.3068 | -1113.0 | -886.5 | |
| 0.00 | 2.53 | 0.00 | 1.30 | 18.02 | 224.31 | 10.73 | 319.01 | 0.2711 | -762.0 | -741.6 | |
| 0.00 | 0.72 | 0.00 | 0.37 | 18.09 | 224.02 | 10.44 | 319.93 | 0.2688 | -853.0 | -772.6 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 18.71 | 223.67 | 10.09 | 322.40 | 0.2731 | -1124.0 | -896.8 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 19.55 | 221.96 | 8.37 | 329.09 | 0.2683 | 717.0 | 561.5 | |
| 0.00 | 2.08 | 0.00 | 1.07 | 19.37 | 221.85 | 8.27 | 329.03 | 0.2648 | 861.0 | 544.9 | |
| 0.00 | 1.81 | 0.00 | 0.93 | 19.09 | 221.51 | 7.93 | 329.49 | 0.2579 | 799.0 | 711.5 | |
| 0.00 | 1.72 | 0.00 | 0.88 | 19.22 | 221.29 | 7.71 | 330.45 | 0.2579 | 879.0 | 682.1 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 18.11 | 220.66 | 7.08 | 330.18 | 0.2365 | 825.0 | 725.6 | |
| 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. | |