SDO HMI 2011-05-05 15:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.64 | 329.02 | 25.17 | 177.65 | 17.97 | 60.94 | 8.89 | 338.25 | 0.3994 | -804.1 | -356.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.35 | 307.85 | 22.85 | 166.15 | 17.81 | 61.23 | 9.18 | 337.49 | 0.3984 | -1421.5 | -423.4 | |
| 4.29 | -1.00 | 2.32 | -1.00 | 18.23 | 60.83 | 8.78 | 338.77 | 0.4022 | -1025.0 | 999999 | |
| 0.00 | 1.16 | 0.00 | 0.63 | 19.51 | 60.44 | 8.40 | 340.74 | 0.4191 | -670.0 | -524.5 | |
| 0.00 | 1.25 | 0.00 | 0.71 | 24.23 | 60.09 | 8.05 | 344.76 | 0.4874 | -727.0 | -560.4 | |
| 0.00 | 0.98 | 0.00 | 0.53 | 19.43 | 59.47 | 7.42 | 342.77 | 0.4131 | -706.0 | -524.8 | |
| 0.00 | 5.90 | 0.00 | 3.16 | 17.78 | 57.80 | 5.75 | 345.40 | 0.3803 | 500.0 | 639.9 | |
| 0.00 | 2.14 | 0.00 | 1.14 | 17.52 | 57.54 | 5.49 | 345.87 | 0.3752 | 764.0 | 678.0 | |
| 0.00 | 1.34 | 0.00 | 0.72 | 17.88 | 57.51 | 5.47 | 346.16 | 0.3807 | 791.0 | 622.3 | |
| 0.00 | 0.63 | 0.00 | 0.34 | 18.50 | 57.50 | 5.46 | 346.59 | 0.3904 | 879.0 | 670.6 | |
| 0.00 | 1.25 | 0.00 | 0.67 | 17.88 | 57.36 | 5.31 | 346.55 | 0.3801 | 821.0 | 702.6 | |
| 0.00 | 1.16 | 0.00 | 0.65 | 23.76 | 55.68 | 3.63 | 352.84 | 0.4671 | 827.0 | 650.9 | |
| 0.00 | 1.16 | 0.00 | 0.62 | 18.85 | 55.50 | 3.45 | 351.57 | 0.3898 | 911.0 | 711.2 | |
| 0.00 | 3.04 | 0.00 | 1.70 | 23.79 | 55.52 | 3.47 | 353.17 | 0.4673 | 759.0 | 658.4 | |
| 0.00 | 1.16 | 0.00 | 0.63 | 19.34 | 54.35 | 2.30 | 354.47 | 0.3953 | 822.0 | 639.8 | |
| 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. | |