SDO HMI 2014-04-22 14:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.79 | 410.83 | 41.64 | 222.86 | 17.75 | 166.64 | 7.60 | 341.96 | 0.4082 | -759.2 | -292.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.72 | 377.64 | 4.20 | 204.99 | 17.90 | 167.52 | 8.48 | 340.11 | 0.4143 | -1106.3 | -382.9 | |
| 1.86 | -1.00 | 1.02 | -1.00 | 18.29 | 167.41 | 8.37 | 340.67 | 0.4196 | -660.6 | 999999 | |
| 60.81 | -1.00 | 32.98 | -1.00 | 17.70 | 167.03 | 7.99 | 341.00 | 0.4087 | -1398.5 | 999999 | |
| 0.89 | -1.00 | 0.48 | -1.00 | 17.99 | 166.57 | 7.53 | 342.26 | 0.4107 | -736.2 | 999999 | |
| 0.00 | 1.24 | 0.00 | 0.67 | 17.60 | 163.56 | 4.52 | 348.92 | 0.3928 | 874.0 | 777.9 | |
| 0.00 | 2.22 | 0.00 | 1.20 | 17.93 | 163.28 | 4.25 | 349.74 | 0.3971 | 920.0 | 790.3 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 17.67 | 163.24 | 4.21 | 349.71 | 0.3929 | 921.0 | 784.5 | |
| 0.00 | 1.33 | 0.00 | 0.72 | 18.29 | 163.10 | 4.06 | 350.33 | 0.4023 | 572.0 | 474.0 | |
| 0.00 | 0.98 | 0.00 | 0.53 | 18.09 | 162.91 | 3.87 | 350.70 | 0.3986 | 670.0 | 591.7 | |
| 0.00 | 2.04 | 0.00 | 1.11 | 19.27 | 162.61 | 3.58 | 351.84 | 0.4166 | 652.0 | 555.4 | |
| 0.00 | 1.24 | 0.00 | 0.67 | 17.96 | 162.49 | 3.45 | 351.64 | 0.3955 | 870.0 | 677.8 | |
| 0.00 | 3.28 | 0.00 | 1.77 | 17.89 | 162.11 | 3.07 | 352.53 | 0.3936 | 816.0 | 719.9 | |
| 0.00 | 1.42 | 0.00 | 0.78 | 19.67 | 161.85 | 2.82 | 353.67 | 0.4213 | 622.0 | 544.3 | |
| 0.00 | 5.06 | 0.00 | 2.71 | 17.27 | 161.37 | 2.33 | 354.14 | 0.3822 | 1130.0 | 839.8 | |
| 0.00 | 1.60 | 0.00 | 0.86 | 17.46 | 161.15 | 2.11 | 354.73 | 0.3850 | 827.0 | 683.6 | |
| 1.69 | 3.02 | 0.91 | 1.62 | 17.85 | 160.40 | 1.36 | 356.67 | 0.3904 | 799.6 | 579.7 | |
| 3.82 | 8.61 | 2.05 | 4.61 | 17.40 | 160.24 | 1.20 | 357.00 | 0.3829 | 1077.4 | 816.9 | |
| 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. | |