SDO HMI 2014-10-08 16:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.95 | 0.00 | 12.29 | -17.07 | 104.74 | 21.16 | 220.64 | 0.5328 | 89.2 | 141.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.02 | 0.00 | 1.20 | -13.73 | 110.68 | 27.09 | 233.19 | 0.5547 | 546.0 | 518.3 | |
| 0.00 | 1.23 | 0.00 | 0.73 | -13.34 | 110.42 | 26.84 | 233.52 | 0.5484 | 848.0 | 682.6 | |
| 0.00 | 2.98 | 0.00 | 1.76 | -13.50 | 110.41 | 26.82 | 233.27 | 0.5496 | 527.0 | 585.6 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -13.78 | 110.44 | 26.86 | 232.88 | 0.5524 | 664.0 | 547.8 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -13.70 | 110.05 | 26.47 | 232.60 | 0.5472 | 729.0 | 647.7 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -18.33 | 108.40 | 24.82 | 224.37 | 0.5720 | 556.0 | 440.3 | |
| 0.00 | 1.40 | 0.00 | 0.82 | -15.45 | 107.25 | 23.67 | 226.92 | 0.5318 | 705.0 | 533.6 | |
| 0.00 | 2.45 | 0.00 | 1.54 | -22.71 | 108.31 | 24.73 | 219.04 | 0.6149 | 672.0 | 537.1 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -17.39 | 101.88 | 18.30 | 217.06 | 0.4991 | -565.0 | -496.6 | |
| 0.00 | 1.49 | 0.00 | 0.85 | -17.06 | 101.81 | 18.23 | 217.38 | 0.4946 | -783.0 | -542.0 | |
| 0.00 | 1.67 | 0.00 | 0.96 | -19.75 | 99.68 | 16.09 | 210.93 | 0.5095 | -605.0 | -380.2 | |
| 0.00 | 0.96 | 0.00 | 0.55 | -19.17 | 98.01 | 14.42 | 208.85 | 0.4894 | -735.0 | -654.7 | |
| 0.00 | 1.40 | 0.00 | 0.79 | -18.57 | 97.92 | 14.34 | 209.34 | 0.4809 | -712.0 | -562.6 | |
| 0.00 | 2.10 | 0.00 | 1.17 | -19.94 | 89.11 | 5.52 | 191.56 | 0.4529 | -598.0 | -537.8 | |
| 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. | |