SDO HMI 2014-01-15 15:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.17 | 408.22 | 39.98 | 214.39 | -16.35 | 12.59 | 15.69 | 231.39 | 0.3333 | 1065.4 | 399.1 | |
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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 | -16.19 | 17.11 | 20.20 | 238.17 | 0.3920 | -817.0 | -529.9 | |
| 0.00 | 0.77 | 0.00 | 0.42 | -20.91 | 15.78 | 18.88 | 226.67 | 0.4173 | 746.0 | 497.3 | |
| 39.78 | 254.59 | 20.98 | 134.27 | -16.55 | 13.32 | 16.42 | 232.17 | 0.3445 | 1326.8 | 384.8 | |
| 4.34 | -3.00 | 2.28 | -3.00 | -16.68 | 12.69 | 15.79 | 230.82 | 0.3377 | 1188.2 | 999999 | |
| 0.00 | 2.13 | 0.00 | 1.11 | -16.21 | 12.24 | 15.33 | 231.20 | 0.3273 | 861.0 | 627.9 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -14.95 | 11.89 | 14.99 | 233.84 | 0.3108 | 886.0 | 658.4 | |
| 0.43 | 138.81 | 0.22 | 72.39 | -15.38 | 11.82 | 14.92 | 232.61 | 0.3139 | 1039.2 | 484.0 | |
| 31.62 | -7.00 | 16.50 | -7.00 | -15.89 | 11.58 | 14.67 | 230.83 | 0.3157 | 1354.9 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.75 | -14.40 | 11.35 | 14.44 | 234.43 | 0.2984 | -746.0 | -519.1 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -18.76 | 11.68 | 14.78 | 224.31 | 0.3473 | 716.0 | 576.2 | |
| 0.00 | 2.04 | 0.00 | 1.08 | -18.86 | 11.56 | 14.66 | 223.89 | 0.3470 | 838.0 | 697.2 | |
| 0.00 | 1.45 | 0.00 | 0.74 | -17.11 | 7.06 | 10.15 | 217.71 | 0.2767 | -754.0 | -618.6 | |
| 0.00 | 2.47 | 0.00 | 1.27 | -17.63 | 6.24 | 9.34 | 214.29 | 0.2756 | -857.0 | -669.4 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -17.35 | 3.79 | 6.89 | 207.33 | 0.2505 | -726.0 | -605.2 | |
| 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. | |