SDO HMI 2014-05-31 03:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.77 | 82.75 | 11.87 | 42.99 | -8.91 | 24.88 | 15.50 | 241.65 | 0.3013 | 609.7 | 505.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.99 | 0.00 | 1.04 | -6.85 | 27.08 | 17.69 | 250.62 | 0.3212 | 583.0 | 433.7 | |
| 1.72 | 5.51 | 0.90 | 2.89 | -9.03 | 26.50 | 17.11 | 243.67 | 0.3256 | 811.6 | 534.5 | |
| 4.97 | 7.05 | 2.60 | 3.69 | -8.72 | 26.38 | 17.00 | 244.40 | 0.3218 | 1016.5 | 833.0 | |
| 0.00 | 1.17 | 0.00 | 0.61 | -8.66 | 25.74 | 16.35 | 243.73 | 0.3118 | 138.0 | 165.0 | |
| 15.27 | 45.89 | 7.95 | 23.89 | -8.94 | 25.43 | 16.05 | 242.50 | 0.3092 | 1197.4 | 725.3 | |
| 0.00 | 2.35 | 0.00 | 1.22 | -9.46 | 25.10 | 15.72 | 240.50 | 0.3083 | 171.0 | 138.0 | |
| 0.00 | 1.08 | 0.00 | 0.56 | -9.46 | 23.92 | 14.54 | 238.60 | 0.2913 | 764.0 | 523.8 | |
| 0.00 | 2.26 | 0.00 | 1.17 | -9.77 | 23.55 | 14.17 | 237.03 | 0.2887 | 984.0 | 761.2 | |
| 0.00 | 1.17 | 0.00 | 0.61 | -9.99 | 23.53 | 14.14 | 236.36 | 0.2903 | 870.0 | 739.2 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -9.86 | 23.24 | 13.85 | 236.18 | 0.2852 | 973.0 | 865.3 | |
| 0.00 | 2.17 | 0.00 | 1.12 | -10.20 | 23.25 | 13.87 | 235.21 | 0.2885 | 937.0 | 779.2 | |
| 0.81 | 3.07 | 0.42 | 1.59 | -10.08 | 22.99 | 13.61 | 235.08 | 0.2838 | 1073.2 | 832.6 | |
| 0.00 | 2.26 | 0.00 | 1.15 | -8.18 | 20.63 | 11.24 | 236.28 | 0.2330 | -721.0 | -601.7 | |
| 0.00 | 1.54 | 0.00 | 0.78 | -8.52 | 20.54 | 11.16 | 234.87 | 0.2350 | -936.0 | -785.4 | |
| 0.00 | 1.08 | 0.00 | 0.55 | -9.19 | 20.47 | 11.08 | 232.37 | 0.2407 | -782.0 | -670.8 | |
| 0.00 | 1.63 | 0.00 | 0.82 | -4.45 | 20.11 | 10.73 | 250.95 | 0.1972 | -822.0 | -668.8 | |
| 0.00 | 1.17 | 0.00 | 0.60 | -8.61 | 20.11 | 10.72 | 233.48 | 0.2299 | -804.0 | -608.6 | |
| 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. | |