SDO HMI 2014-04-24 11:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.23 | 354.19 | 34.58 | 225.46 | 17.87 | 166.30 | 32.04 | 306.49 | 0.6301 | -778.8 | -309.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.23 | 336.30 | 34.58 | 214.42 | 17.87 | 166.44 | 32.18 | 306.37 | 0.6317 | -1256.1 | -349.1 | |
| 0.00 | 3.56 | 0.00 | 2.22 | 17.31 | 164.77 | 30.51 | 307.02 | 0.6092 | -342.0 | -121.9 | |
| 0.00 | 1.87 | 0.00 | 1.16 | 17.49 | 164.55 | 30.29 | 307.46 | 0.6082 | -369.0 | -350.9 | |
| 0.00 | 1.07 | 0.00 | 0.66 | 17.16 | 164.34 | 30.08 | 307.19 | 0.6033 | 676.0 | 580.4 | |
| 0.00 | 0.98 | 0.00 | 0.60 | 17.55 | 163.47 | 29.20 | 308.51 | 0.5967 | 622.0 | 515.8 | |
| 0.00 | 1.24 | 0.00 | 0.77 | 17.74 | 163.39 | 29.13 | 308.84 | 0.5974 | 564.0 | 504.1 | |
| 0.00 | 2.31 | 0.00 | 1.42 | 17.86 | 163.20 | 28.93 | 309.19 | 0.5963 | 737.0 | 653.6 | |
| 0.00 | 1.07 | 0.00 | 0.66 | 17.98 | 163.04 | 28.77 | 309.51 | 0.5956 | 704.0 | 499.4 | |
| 0.00 | 0.62 | 0.00 | 0.38 | 18.41 | 162.97 | 28.70 | 310.15 | 0.5984 | 535.0 | 504.9 | |
| 0.00 | 1.96 | 0.00 | 1.20 | 18.17 | 162.71 | 28.44 | 310.07 | 0.5936 | 796.0 | 650.1 | |
| 0.00 | 0.98 | 0.00 | 0.60 | 18.59 | 162.71 | 28.45 | 310.64 | 0.5972 | 653.0 | 544.1 | |
| 0.00 | 0.80 | 0.00 | 0.49 | 17.96 | 162.49 | 28.23 | 310.00 | 0.5895 | 714.0 | 626.7 | |
| 0.00 | 1.16 | 0.00 | 0.71 | 18.12 | 162.45 | 28.18 | 310.27 | 0.5904 | 707.0 | 621.0 | |
| 0.00 | 0.27 | 0.00 | 0.17 | 19.83 | 162.40 | 28.14 | 312.57 | 0.6047 | 385.0 | 351.0 | |
| 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. | |