SDO HMI 2014-01-12 13:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.23 | 134.34 | 37.17 | 69.11 | -17.90 | 29.80 | -7.71 | 151.79 | 0.2701 | 63.8 | 199.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.82 | 70.63 | 19.38 | 36.21 | -17.67 | 30.84 | -6.67 | 154.51 | 0.2583 | 1163.9 | 596.9 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -17.09 | 30.64 | -6.86 | 152.80 | 0.2511 | 826.0 | 677.1 | |
| 0.76 | 5.95 | 0.39 | 3.06 | -18.24 | 30.32 | -7.19 | 153.82 | 0.2707 | 786.3 | 565.5 | |
| 0.00 | 2.12 | 0.00 | 1.09 | -17.75 | 30.15 | -7.36 | 152.43 | 0.2647 | 58.0 | 147.6 | |
| 0.00 | 1.44 | 0.00 | 0.74 | -17.36 | 30.01 | -7.50 | 151.24 | 0.2600 | 824.0 | 567.6 | |
| 0.00 | 1.44 | 0.00 | 0.74 | -17.66 | 29.94 | -7.57 | 151.58 | 0.2651 | 665.0 | 519.5 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -18.47 | 29.18 | -8.33 | 150.80 | 0.2830 | -620.0 | -452.2 | |
| 0.00 | 2.46 | 0.00 | 1.27 | -18.17 | 29.13 | -8.38 | 150.10 | 0.2790 | -660.0 | -399.7 | |
| 0.42 | 3.48 | 0.22 | 1.80 | -18.56 | 28.95 | -8.56 | 150.32 | 0.2861 | -955.0 | -784.4 | |
| 0.00 | 0.93 | 0.00 | 0.48 | -18.74 | 28.69 | -8.82 | 149.92 | 0.2909 | -656.0 | -537.4 | |
| 1.53 | 42.24 | 0.79 | 21.84 | -18.40 | 28.52 | -8.99 | 148.81 | 0.2876 | -838.9 | -752.9 | |
| 0.00 | 1.61 | 0.00 | 0.83 | -17.86 | 28.52 | -8.99 | 147.74 | 0.2799 | -1010.0 | -881.1 | |
| 20.74 | -11.00 | 10.73 | -11.00 | -18.28 | 28.15 | -9.36 | 147.55 | 0.2891 | -1046.3 | 999999 | |
| 10.96 | -11.00 | 5.66 | -11.00 | -17.97 | 28.14 | -9.37 | 146.91 | 0.2850 | -1238.6 | 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. | |