SDO HMI 2014-03-15 01:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.36 | 165.50 | 50.97 | 195.63 | 11.26 | 10.26 | 62.71 | 286.00 | 0.9083 | -84.4 | -108.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.73 | 96.00 | 17.12 | 118.50 | 11.76 | 11.71 | 64.16 | 286.17 | 0.9192 | -366.4 | -223.6 | |
| 2.87 | -1.00 | 3.50 | -1.00 | 11.46 | 11.23 | 63.68 | 285.97 | 0.9155 | -567.7 | 999999 | |
| 0.00 | 1.56 | 0.00 | 1.85 | 10.52 | 10.65 | 63.11 | 285.11 | 0.9100 | 119.0 | 47.1 | |
| 3.82 | -1.00 | 4.60 | -1.00 | 11.59 | 10.81 | 63.26 | 286.22 | 0.9128 | -654.1 | 999999 | |
| 2.78 | -1.00 | 3.36 | -1.00 | 11.88 | 10.86 | 63.31 | 286.51 | 0.9137 | -505.3 | 999999 | |
| 2.26 | -1.00 | 2.65 | -1.00 | 11.62 | 10.21 | 62.66 | 286.40 | 0.9088 | -488.4 | 999999 | |
| 0.00 | 0.96 | 0.00 | 1.10 | 11.17 | 9.83 | 62.28 | 286.02 | 0.9054 | -285.0 | -255.8 | |
| 0.00 | 2.52 | 0.00 | 2.84 | 10.31 | 9.32 | 61.77 | 285.21 | 0.9002 | 10.0 | 28.2 | |
| 7.73 | 34.06 | 8.62 | 38.29 | 10.79 | 8.91 | 61.36 | 285.84 | 0.8980 | 200.8 | -207.9 | |
| 2.35 | -9.00 | 2.60 | -9.00 | 10.43 | 8.79 | 61.24 | 285.49 | 0.8965 | 424.4 | 999999 | |
| 7.82 | 26.76 | 8.52 | 29.15 | 10.32 | 8.31 | 60.76 | 285.48 | 0.8927 | 697.7 | 420.1 | |
| 0.00 | 1.30 | 0.00 | 1.44 | 11.27 | 8.51 | 60.97 | 286.47 | 0.8960 | 23.0 | 36.7 | |
| 0.00 | 1.04 | 0.00 | 1.10 | 11.42 | 7.02 | 59.47 | 287.03 | 0.8850 | 343.0 | 312.8 | |
| 0.00 | 1.30 | 0.00 | 1.36 | 11.14 | 6.75 | 59.20 | 286.80 | 0.8823 | 464.0 | 363.0 | |
| 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. | |