SDO HMI 2014-05-18 11:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.71 | 249.51 | 41.13 | 133.88 | -16.58 | 194.72 | 17.72 | 229.47 | 0.3849 | 133.1 | 63.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.64 | -17.69 | 197.33 | 20.33 | 231.01 | 0.4277 | 754.0 | 634.4 | |
| 33.81 | 110.86 | 18.35 | 60.14 | -17.39 | 196.11 | 19.12 | 229.95 | 0.4100 | 1099.7 | 407.2 | |
| 3.69 | 12.32 | 1.99 | 6.64 | -16.49 | 195.72 | 18.72 | 231.21 | 0.3965 | 1095.1 | 826.5 | |
| 0.00 | 2.34 | 0.00 | 1.26 | -16.37 | 195.24 | 18.24 | 230.77 | 0.3894 | 735.0 | 632.9 | |
| 1.35 | 8.99 | 0.72 | 4.83 | -16.46 | 195.05 | 18.05 | 230.29 | 0.3880 | 1165.1 | 796.5 | |
| 0.63 | -5.00 | 0.34 | -5.00 | -16.62 | 194.80 | 17.80 | 229.59 | 0.3864 | 960.9 | 999999 | |
| 0.00 | 1.80 | 0.00 | 0.96 | -16.72 | 194.34 | 17.35 | 228.68 | 0.3818 | 340.0 | 317.6 | |
| 2.79 | 110.41 | 1.48 | 58.57 | -15.76 | 193.86 | 16.86 | 229.96 | 0.3662 | -774.0 | -517.2 | |
| 5.57 | -8.00 | 2.96 | -8.00 | -15.88 | 193.64 | 16.64 | 229.33 | 0.3648 | -914.5 | 999999 | |
| 2.79 | -8.00 | 1.48 | -8.00 | -15.89 | 193.41 | 16.41 | 228.95 | 0.3620 | -1006.9 | 999999 | |
| 1.17 | -8.00 | 0.62 | -8.00 | -15.64 | 193.39 | 16.39 | 229.46 | 0.3592 | -963.3 | 999999 | |
| 12.14 | -8.00 | 6.44 | -8.00 | -16.08 | 193.10 | 16.10 | 228.01 | 0.3601 | -983.2 | 999999 | |
| 12.77 | -8.00 | 6.75 | -8.00 | -15.42 | 192.98 | 15.98 | 229.25 | 0.3519 | -1287.9 | 999999 | |
| 0.00 | 1.62 | 0.00 | 0.84 | -15.25 | 187.12 | 10.13 | 217.03 | 0.2830 | 790.0 | 690.7 | |
| 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. | |