SDO HMI 2011-10-10 03:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.10 | 56.71 | 15.60 | 30.51 | 20.72 | 111.39 | -18.28 | 49.03 | 0.3907 | 5.9 | 384.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.31 | 0.00 | 0.71 | 21.83 | 111.85 | -17.81 | 46.06 | 0.3960 | 858.0 | 664.5 | |
| 0.00 | 3.86 | 0.00 | 2.09 | 22.39 | 111.75 | -17.92 | 45.15 | 0.4030 | 861.0 | 725.7 | |
| 18.06 | 22.00 | 9.65 | 11.76 | 20.01 | 111.98 | -17.69 | 49.62 | 0.3764 | -957.8 | -332.0 | |
| 0.00 | 2.10 | 0.00 | 1.15 | 24.51 | 111.20 | -18.46 | 42.13 | 0.4314 | 839.0 | 576.4 | |
| 0.00 | 1.58 | 0.00 | 0.86 | 23.06 | 111.17 | -18.49 | 44.73 | 0.4164 | 906.0 | 820.4 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 23.44 | 111.09 | -18.58 | 44.18 | 0.4212 | 774.0 | 654.9 | |
| 0.00 | 1.49 | 0.00 | 0.80 | 20.82 | 111.31 | -18.36 | 48.89 | 0.3924 | 754.0 | 491.8 | |
| 1.75 | 20.34 | 0.94 | 10.97 | 20.48 | 111.15 | -18.52 | 49.83 | 0.3910 | 975.3 | 660.9 | |
| 0.96 | -8.00 | 0.52 | -8.00 | 20.72 | 111.01 | -18.65 | 49.51 | 0.3950 | 836.5 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 19.83 | 111.13 | -18.54 | 51.23 | 0.3853 | -745.0 | -616.3 | |
| 6.40 | -8.00 | 3.45 | -8.00 | 20.56 | 110.76 | -18.90 | 50.20 | 0.3965 | 1030.8 | 999999 | |
| 0.00 | 2.10 | 0.00 | 1.13 | 19.66 | 110.88 | -18.79 | 51.93 | 0.3869 | -659.0 | -476.8 | |
| 1.93 | -8.00 | 1.04 | -8.00 | 20.57 | 110.39 | -19.27 | 50.67 | 0.4013 | 851.7 | 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. | |