SDO HMI 2014-11-25 02:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.10 | 60.98 | 8.52 | 32.26 | 4.69 | 157.90 | -20.40 | 81.05 | 0.3533 | 115.6 | -13.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.37 | 9.94 | 0.71 | 5.18 | 4.08 | 160.21 | -18.09 | 81.97 | 0.3142 | -1166.5 | -799.3 | |
| 3.77 | -1.00 | 1.97 | -1.00 | 4.28 | 160.05 | -18.25 | 81.39 | 0.3173 | -944.7 | 999999 | |
| 0.00 | 6.85 | 0.00 | 3.59 | 4.16 | 159.37 | -18.94 | 82.04 | 0.3283 | -916.0 | -722.6 | |
| 0.00 | 1.71 | 0.00 | 0.90 | 3.92 | 159.28 | -19.02 | 82.79 | 0.3293 | -931.0 | -798.5 | |
| 0.00 | 0.77 | 0.00 | 0.40 | 4.43 | 159.27 | -19.04 | 81.28 | 0.3305 | -742.0 | -615.1 | |
| 1.11 | 3.85 | 0.59 | 2.03 | 5.02 | 159.00 | -19.30 | 79.64 | 0.3363 | -986.2 | -804.3 | |
| 1.11 | 4.54 | 0.59 | 2.40 | 5.22 | 158.14 | -20.16 | 79.46 | 0.3507 | -978.8 | -798.3 | |
| 0.34 | 6.08 | 0.18 | 3.21 | 4.50 | 158.00 | -20.30 | 81.54 | 0.3512 | 891.2 | 391.5 | |
| 0.00 | 2.91 | 0.00 | 1.54 | 4.71 | 157.74 | -20.56 | 81.05 | 0.3559 | 94.0 | 129.0 | |
| 4.54 | 9.34 | 2.42 | 4.98 | 5.77 | 156.78 | -21.52 | 78.58 | 0.3740 | 1040.2 | 773.9 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 4.55 | 156.79 | -21.51 | 81.82 | 0.3709 | 699.0 | 481.7 | |
| 0.00 | 1.20 | 0.00 | 0.64 | 4.73 | 156.66 | -21.64 | 81.39 | 0.3734 | 851.0 | 627.3 | |
| 1.97 | 4.20 | 1.05 | 2.24 | 5.14 | 156.49 | -21.82 | 80.36 | 0.3771 | 1072.0 | 829.4 | |
| 0.43 | 1.54 | 0.23 | 0.83 | 4.10 | 156.04 | -22.26 | 83.24 | 0.3822 | 1036.8 | 874.1 | |
| 1.46 | 7.28 | 0.78 | 3.91 | 4.15 | 155.39 | -22.91 | 83.27 | 0.3927 | 940.9 | 758.0 | |
| 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. | |