SDO HMI 2014-10-10 11:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.71 | 0.00 | 10.73 | 13.23 | 93.85 | 33.90 | 285.81 | 0.5641 | 0.1 | 32.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.49 | 0.00 | 1.02 | 9.91 | 103.94 | 44.00 | 277.88 | 0.6931 | -593.0 | -464.4 | |
| 0.00 | 1.23 | 0.00 | 0.83 | 10.37 | 103.01 | 43.06 | 278.60 | 0.6816 | -578.0 | -522.9 | |
| 0.00 | 1.49 | 0.00 | 0.99 | 11.04 | 101.80 | 41.85 | 279.66 | 0.6666 | -502.0 | -409.5 | |
| 0.00 | 0.79 | 0.00 | 0.52 | 11.16 | 101.33 | 41.38 | 279.89 | 0.6607 | -525.0 | -495.2 | |
| 0.00 | 0.61 | 0.00 | 0.39 | 11.82 | 98.72 | 38.78 | 281.21 | 0.6272 | -634.0 | -558.3 | |
| 0.00 | 0.79 | 0.00 | 0.50 | 12.44 | 98.55 | 38.61 | 282.21 | 0.6257 | -731.0 | -588.3 | |
| 0.00 | 1.05 | 0.00 | 0.65 | 7.75 | 96.48 | 36.53 | 274.68 | 0.5940 | -645.0 | -577.5 | |
| 0.00 | 1.14 | 0.00 | 0.69 | 12.28 | 94.44 | 34.49 | 282.69 | 0.5693 | -669.0 | -498.8 | |
| 0.00 | 1.14 | 0.00 | 0.66 | 13.95 | 91.24 | 31.29 | 286.60 | 0.5281 | 656.0 | 464.3 | |
| 0.00 | 1.23 | 0.00 | 0.70 | 12.40 | 89.07 | 29.12 | 284.35 | 0.4926 | 545.0 | 522.2 | |
| 0.00 | 0.70 | 0.00 | 0.40 | 16.31 | 88.10 | 28.16 | 292.54 | 0.4923 | 452.0 | 374.9 | |
| 0.00 | 2.28 | 0.00 | 1.28 | 15.33 | 86.97 | 27.03 | 291.23 | 0.4721 | 869.0 | 747.5 | |
| 0.00 | 1.67 | 0.00 | 0.94 | 19.76 | 85.32 | 25.37 | 301.22 | 0.4735 | 759.0 | 606.5 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 16.98 | 84.36 | 24.42 | 296.41 | 0.4433 | 835.0 | 707.6 | |
| 0.00 | 0.96 | 0.00 | 0.53 | 16.65 | 82.72 | 22.77 | 297.08 | 0.4182 | 762.0 | 663.5 | |
| 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. | |