SDO HMI 2014-04-22 18:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70.82 | 415.31 | 38.63 | 226.57 | 17.75 | 166.56 | 9.73 | 337.39 | 0.4200 | -687.1 | -295.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.21 | 377.04 | 36.15 | 205.91 | 17.73 | 167.03 | 10.20 | 336.32 | 0.4219 | -1385.1 | -398.8 | |
| 0.00 | 1.15 | 0.00 | 0.63 | 18.52 | 165.50 | 8.67 | 340.23 | 0.4246 | -722.0 | -596.1 | |
| 0.00 | 1.60 | 0.00 | 0.86 | 17.91 | 163.30 | 6.47 | 344.57 | 0.4047 | 1011.0 | 773.3 | |
| 0.00 | 0.80 | 0.00 | 0.43 | 17.71 | 163.26 | 6.43 | 344.52 | 0.4015 | 744.0 | 553.0 | |
| 0.00 | 3.64 | 0.00 | 1.98 | 18.60 | 163.07 | 6.24 | 345.54 | 0.4143 | 750.0 | 657.0 | |
| 0.00 | 0.80 | 0.00 | 0.43 | 18.30 | 162.93 | 6.10 | 345.66 | 0.4092 | 781.0 | 683.3 | |
| 0.00 | 1.42 | 0.00 | 0.77 | 17.91 | 162.89 | 6.06 | 345.51 | 0.4029 | 1038.0 | 930.5 | |
| 0.00 | 1.07 | 0.00 | 0.58 | 18.17 | 162.70 | 5.87 | 346.09 | 0.4063 | 699.0 | 649.5 | |
| 0.00 | 2.93 | 0.00 | 1.60 | 19.29 | 162.62 | 5.79 | 346.95 | 0.4232 | 677.0 | 529.0 | |
| 0.00 | 1.69 | 0.00 | 0.91 | 17.94 | 162.57 | 5.74 | 346.26 | 0.4022 | 909.0 | 681.7 | |
| 0.00 | 0.71 | 0.00 | 0.38 | 18.26 | 162.48 | 5.65 | 346.65 | 0.4069 | 817.0 | 655.1 | |
| 0.00 | 2.22 | 0.00 | 1.20 | 17.90 | 162.25 | 5.42 | 346.98 | 0.4004 | 970.0 | 799.8 | |
| 0.00 | 1.42 | 0.00 | 0.76 | 17.41 | 161.98 | 5.15 | 347.32 | 0.3918 | 847.0 | 681.9 | |
| 0.00 | 1.60 | 0.00 | 0.88 | 20.07 | 161.45 | 4.62 | 349.86 | 0.4318 | 710.0 | 528.6 | |
| 0.00 | 5.50 | 0.00 | 2.96 | 17.34 | 161.31 | 4.48 | 348.88 | 0.3885 | 937.0 | 838.6 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 17.70 | 160.85 | 4.02 | 350.18 | 0.3928 | 612.0 | 521.0 | |
| 1.15 | 2.40 | 0.62 | 1.29 | 17.79 | 160.41 | 3.57 | 351.28 | 0.3931 | 791.8 | 639.6 | |
| 3.46 | 8.17 | 1.86 | 4.38 | 17.33 | 160.24 | 3.41 | 351.50 | 0.3854 | 1049.5 | 791.6 | |
| 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. | |