SDO HMI 2014-01-13 20:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.78 | 221.74 | 37.09 | 114.63 | -17.87 | 30.19 | 9.71 | 214.27 | 0.2855 | 165.1 | 88.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.89 | 117.84 | 12.93 | 61.16 | -18.13 | 31.56 | 11.08 | 217.45 | 0.3018 | 1188.3 | 442.6 | |
| 3.99 | -1.00 | 2.07 | -1.00 | -17.31 | 31.32 | 10.84 | 218.65 | 0.2889 | 1259.2 | 999999 | |
| 7.65 | -1.00 | 3.96 | -1.00 | -17.62 | 31.18 | 10.71 | 217.62 | 0.2914 | 1141.1 | 999999 | |
| 1.70 | -1.00 | 0.88 | -1.00 | -18.29 | 31.07 | 10.59 | 215.89 | 0.2989 | 841.2 | 999999 | |
| 0.85 | -1.00 | 0.44 | -1.00 | -17.56 | 30.83 | 10.36 | 216.85 | 0.2871 | 1042.1 | 999999 | |
| 0.00 | 1.61 | 0.00 | 0.83 | -17.38 | 30.51 | 10.03 | 216.38 | 0.2815 | 1023.0 | 789.6 | |
| 0.00 | 1.87 | 0.00 | 0.97 | -18.08 | 30.52 | 10.04 | 214.91 | 0.2909 | 729.0 | 590.5 | |
| 0.00 | 3.31 | 0.00 | 1.71 | -17.11 | 30.40 | 9.92 | 216.70 | 0.2769 | 955.0 | 728.0 | |
| 0.00 | 4.67 | 0.00 | 2.42 | -18.26 | 30.24 | 9.77 | 213.81 | 0.2908 | 737.0 | 745.1 | |
| 0.00 | 1.10 | 0.00 | 0.57 | -18.36 | 29.53 | 9.05 | 211.66 | 0.2857 | -691.0 | -591.2 | |
| 2.55 | 53.19 | 1.31 | 27.38 | -17.43 | 29.26 | 8.78 | 212.79 | 0.2702 | -1096.6 | -502.4 | |
| 13.93 | -11.00 | 7.17 | -11.00 | -17.82 | 29.00 | 8.52 | 211.21 | 0.2734 | -1114.4 | 999999 | |
| 0.93 | 2.21 | 0.48 | 1.13 | -17.68 | 28.43 | 7.95 | 209.79 | 0.2665 | -1024.9 | -860.9 | |
| 15.29 | 35.94 | 7.85 | 18.46 | -17.86 | 27.90 | 7.43 | 207.81 | 0.2649 | -1179.8 | -481.2 | |
| 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. | |