| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.90 | 130.28 | 16.60 | 80.63 | -8.77 | 24.94 | -36.28 | 103.01 | 0.6022 | 630.9 | 378.4 | |
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back to the solar disc SDO HMI 2014-05-27 05:00:39 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.56 | 118.48 | 6.50 | 73.02 | -8.92 | 25.43 | -35.79 | 103.38 | 0.5960 | 1136.7 | 432.4 | |
| 0.00 | 0.63 | 0.00 | 0.39 | -8.16 | 25.36 | -35.86 | 102.09 | 0.5952 | 628.0 | 465.6 | |
| 10.65 | -1.00 | 6.57 | -1.00 | -8.77 | 25.26 | -35.96 | 103.08 | 0.5980 | 1001.5 | 999999 | |
| 2.71 | -1.00 | 1.68 | -1.00 | -8.79 | 24.99 | -36.23 | 103.05 | 0.6018 | 809.8 | 999999 | |
| 2.98 | -1.00 | 1.85 | -1.00 | -8.79 | 24.72 | -36.50 | 102.96 | 0.6054 | 781.6 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.45 | -8.48 | 24.37 | -36.85 | 102.36 | 0.6094 | 555.0 | 427.9 | |
| 0.00 | 3.43 | 0.00 | 2.14 | -9.06 | 24.22 | -36.99 | 103.27 | 0.6127 | -187.0 | -70.3 | |
| 0.00 | 0.99 | 0.00 | 0.62 | -8.78 | 24.26 | -36.96 | 102.83 | 0.6116 | 500.0 | 423.0 | |
| 0.00 | 1.44 | 0.00 | 0.90 | -7.86 | 24.01 | -37.20 | 101.27 | 0.6130 | 782.0 | 651.1 | |
| 0.00 | 1.26 | 0.00 | 0.79 | -4.38 | 23.57 | -37.64 | 95.53 | 0.6140 | -560.0 | -440.4 | |
| 0.00 | 0.99 | 0.00 | 0.67 | -9.30 | 19.23 | -41.98 | 102.42 | 0.6783 | -625.0 | -510.7 | |
| 0.00 | 1.35 | 0.00 | 0.93 | -8.17 | 17.71 | -43.50 | 100.50 | 0.6953 | -517.0 | -399.0 | |
| 0.00 | 0.45 | 0.00 | 0.31 | -8.32 | 17.65 | -43.57 | 100.70 | 0.6963 | -244.0 | -277.0 | |
| 0.00 | 0.54 | 0.00 | 0.41 | -8.39 | 12.52 | -48.70 | 100.03 | 0.7570 | -324.0 | -222.3 | |
| 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. | |