SDO HMI 2014-04-02 10:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.51 | 84.40 | 29.97 | 57.12 | 16.89 | 28.86 | -36.40 | 56.50 | 0.6828 | -156.4 | 138.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.81 | 16.53 | 30.81 | -34.45 | 55.57 | 0.6598 | -712.0 | -615.6 | |
| 2.55 | 13.79 | 1.67 | 9.05 | 15.98 | 30.81 | -34.45 | 56.30 | 0.6561 | -848.5 | -559.2 | |
| 4.65 | -2.00 | 3.06 | -2.00 | 15.84 | 30.53 | -34.73 | 56.69 | 0.6581 | -773.1 | 999999 | |
| 24.15 | 30.74 | 16.01 | 20.37 | 16.60 | 30.23 | -35.04 | 55.92 | 0.6666 | -739.9 | -361.7 | |
| 0.00 | 1.32 | 0.00 | 0.88 | 15.81 | 29.47 | -35.80 | 57.49 | 0.6696 | -573.0 | -467.7 | |
| 0.00 | 1.67 | 0.00 | 1.12 | 16.78 | 29.07 | -36.19 | 56.53 | 0.6801 | 325.0 | 378.6 | |
| 0.00 | 1.05 | 0.00 | 0.72 | 17.37 | 28.50 | -36.76 | 56.17 | 0.6899 | 269.0 | 188.8 | |
| 0.00 | 4.39 | 0.00 | 3.04 | 18.19 | 27.99 | -37.27 | 55.51 | 0.7004 | 562.0 | 596.0 | |
| 1.14 | 3.60 | 0.78 | 2.47 | 17.43 | 28.13 | -37.13 | 56.35 | 0.6941 | 786.4 | 658.0 | |
| 0.61 | 1.76 | 0.43 | 1.22 | 17.94 | 27.81 | -37.45 | 55.93 | 0.7007 | 675.9 | 606.2 | |
| 0.00 | 1.05 | 0.00 | 0.73 | 17.45 | 27.85 | -37.41 | 56.52 | 0.6972 | 625.0 | 493.2 | |
| 0.00 | 0.88 | 0.00 | 0.60 | 15.93 | 27.45 | -37.81 | 58.72 | 0.6921 | 600.0 | 483.6 | |
| 2.37 | 19.32 | 1.66 | 13.57 | 17.75 | 26.86 | -38.40 | 56.81 | 0.7093 | 718.9 | 495.3 | |
| 7.99 | -13.00 | 5.62 | -13.00 | 17.52 | 26.52 | -38.75 | 57.32 | 0.7114 | 700.3 | 999999 | |
| 1.05 | -13.00 | 0.74 | -13.00 | 17.78 | 26.45 | -38.82 | 57.04 | 0.7137 | 372.2 | 999999 | |
| 0.00 | 1.58 | 0.00 | 1.11 | 17.00 | 26.00 | -39.27 | 58.29 | 0.7138 | 723.0 | 577.9 | |
| 0.00 | 2.02 | 0.00 | 1.43 | 17.02 | 25.79 | -39.47 | 58.40 | 0.7160 | 575.0 | 471.6 | |
| 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. | |