SDO HMI 2014-10-12 00:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.90 | 0.00 | 9.98 | 13.72 | 58.15 | 18.56 | 294.69 | 0.3409 | 206.1 | 183.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.36 | 0.00 | 1.32 | 11.79 | 66.95 | 27.36 | 283.80 | 0.4652 | -805.0 | -623.4 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 12.27 | 63.10 | 23.51 | 286.55 | 0.4084 | -802.0 | -722.1 | |
| 0.00 | 0.61 | 0.00 | 0.33 | 18.29 | 60.76 | 21.17 | 302.41 | 0.4079 | -753.0 | -632.9 | |
| 0.00 | 1.31 | 0.00 | 0.71 | 18.51 | 60.59 | 21.00 | 303.08 | 0.4073 | -576.0 | -495.3 | |
| 0.00 | 1.66 | 0.00 | 0.88 | 12.73 | 59.80 | 20.21 | 289.84 | 0.3599 | 858.0 | 751.3 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 17.67 | 60.08 | 20.49 | 301.79 | 0.3941 | -690.0 | -553.1 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 16.78 | 59.44 | 19.85 | 300.44 | 0.3788 | -751.0 | -581.2 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 13.46 | 58.82 | 19.23 | 292.64 | 0.3486 | 735.0 | 576.3 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 13.66 | 55.38 | 15.79 | 297.09 | 0.2984 | 710.0 | 618.5 | |
| 0.00 | 1.31 | 0.00 | 0.68 | 13.54 | 55.25 | 15.66 | 296.91 | 0.2955 | 843.0 | 706.2 | |
| 0.00 | 1.49 | 0.00 | 0.77 | 13.12 | 55.22 | 15.63 | 295.63 | 0.2923 | 866.0 | 584.6 | |
| 0.00 | 1.31 | 0.00 | 0.68 | 13.35 | 54.59 | 15.01 | 297.21 | 0.2845 | 861.0 | 727.9 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 11.15 | 53.65 | 14.06 | 290.88 | 0.2562 | 933.0 | 790.0 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 13.36 | 53.29 | 13.70 | 299.24 | 0.2653 | 846.0 | 725.9 | |
| 0.00 | 1.93 | 0.00 | 0.98 | 11.81 | 51.23 | 11.64 | 297.17 | 0.2231 | 817.0 | 575.2 | |
| 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. | |