SDO HMI 2014-04-05 06:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.78 | 165.50 | 16.70 | 89.74 | 17.60 | 30.06 | 2.19 | 354.89 | 0.4097 | -38.6 | -400.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.16 | 138.22 | 7.69 | 74.96 | 17.63 | 30.94 | 3.07 | 352.82 | 0.4106 | -1240.2 | -509.8 | |
| 1.23 | -1.00 | 0.67 | -1.00 | 17.47 | 30.65 | 2.79 | 353.44 | 0.4074 | -1417.2 | 999999 | |
| 1.23 | -1.00 | 0.67 | -1.00 | 17.90 | 30.57 | 2.70 | 353.76 | 0.4141 | -794.6 | 999999 | |
| 1.41 | -1.00 | 0.76 | -1.00 | 17.57 | 30.53 | 2.66 | 353.76 | 0.4088 | -1027.9 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 17.17 | 29.68 | 1.81 | 355.67 | 0.4012 | -178.0 | -113.1 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 15.77 | 29.44 | 1.57 | 355.98 | 0.3784 | -712.0 | -509.7 | |
| 0.00 | 1.41 | 0.00 | 0.76 | 16.42 | 27.17 | -0.70 | 1.74 | 0.3882 | 787.0 | 531.8 | |
| 0.00 | 1.41 | 0.00 | 0.76 | 16.95 | 26.10 | -1.77 | 4.28 | 0.3976 | 830.0 | 634.9 | |
| 7.74 | 15.84 | 4.19 | 8.57 | 17.34 | 25.72 | -2.15 | 5.10 | 0.4044 | 1050.8 | 776.4 | |
| 0.00 | 1.32 | 0.00 | 0.72 | 18.16 | 25.61 | -2.25 | 5.16 | 0.4176 | 611.0 | 499.4 | |
| 0.00 | 1.85 | 0.00 | 1.00 | 17.67 | 25.62 | -2.25 | 5.26 | 0.4098 | 722.0 | 599.6 | |
| 5.01 | -9.00 | 2.72 | -9.00 | 17.41 | 25.47 | -2.40 | 5.68 | 0.4058 | 1066.1 | 999999 | |
| 0.00 | 2.29 | 0.00 | 1.25 | 18.30 | 25.36 | -2.51 | 5.70 | 0.4201 | 707.0 | 607.6 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 18.53 | 25.04 | -2.83 | 6.36 | 0.4243 | 778.0 | 588.8 | |
| 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. | |