SDO HMI 2014-01-15 14:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74.31 | 391.35 | 38.89 | 204.91 | -16.29 | 12.53 | 15.08 | 230.46 | 0.3251 | 1002.1 | 415.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.02 | 0.00 | 0.55 | -17.27 | 18.24 | 20.78 | 236.48 | 0.4082 | 747.0 | 614.1 | |
| 0.00 | 0.94 | 0.00 | 0.50 | -16.21 | 17.13 | 19.68 | 237.51 | 0.3851 | -925.0 | -669.8 | |
| 37.49 | 238.30 | 19.72 | 125.34 | -16.53 | 13.32 | 15.87 | 231.31 | 0.3374 | 1359.3 | 417.9 | |
| 4.85 | -3.00 | 2.54 | -3.00 | -16.67 | 12.70 | 15.24 | 229.91 | 0.3307 | 1170.1 | 999999 | |
| 1.45 | 141.55 | 0.75 | 73.64 | -15.36 | 11.93 | 14.48 | 231.85 | 0.3079 | 1019.4 | 480.5 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -15.00 | 11.91 | 14.45 | 232.77 | 0.3041 | 778.0 | 593.3 | |
| 30.52 | -5.00 | 15.88 | -5.00 | -15.90 | 11.56 | 14.10 | 229.73 | 0.3086 | 1365.5 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -14.44 | 11.37 | 13.91 | 233.33 | 0.2916 | -727.0 | -504.0 | |
| 0.00 | 1.02 | 0.00 | 0.54 | -18.87 | 11.66 | 14.21 | 223.01 | 0.3420 | 751.0 | 652.8 | |
| 0.00 | 1.45 | 0.00 | 0.74 | -16.30 | 7.47 | 10.02 | 219.28 | 0.2649 | -818.0 | -585.1 | |
| 0.00 | 1.70 | 0.00 | 0.87 | -17.64 | 6.29 | 8.83 | 212.84 | 0.2711 | -830.0 | -691.8 | |
| 0.00 | 1.45 | 0.00 | 0.72 | -9.71 | 4.34 | 6.89 | 232.76 | 0.1492 | -826.0 | -666.8 | |
| 0.00 | 1.28 | 0.00 | 0.65 | -18.18 | 2.94 | 5.48 | 201.09 | 0.2535 | -759.0 | -540.4 | |
| 0.00 | 0.34 | 0.00 | 0.17 | -14.87 | 2.33 | 4.87 | 204.66 | 0.1977 | -628.0 | -520.5 | |
| 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. | |