SDO HMI 2014-04-02 02:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.49 | 43.73 | 10.69 | 31.88 | 16.95 | 28.17 | -41.47 | 59.64 | 0.7362 | 176.1 | -21.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.79 | 10.01 | 0.55 | 7.03 | 15.89 | 30.05 | -39.60 | 59.85 | 0.7112 | -811.6 | -554.5 | |
| 0.00 | 1.23 | 0.00 | 0.87 | 16.82 | 29.70 | -39.95 | 58.90 | 0.7201 | -527.0 | -462.1 | |
| 3.78 | -1.00 | 2.66 | -1.00 | 15.68 | 29.81 | -39.83 | 60.26 | 0.7126 | -827.3 | 999999 | |
| 0.00 | 4.21 | 0.00 | 3.01 | 17.00 | 29.49 | -40.16 | 58.81 | 0.7232 | -667.0 | -580.9 | |
| 0.00 | 1.76 | 0.00 | 1.26 | 17.25 | 29.18 | -40.47 | 58.69 | 0.7278 | -268.0 | -306.5 | |
| 0.00 | 0.61 | 0.00 | 0.44 | 15.81 | 29.46 | -40.19 | 60.31 | 0.7170 | -41.0 | -108.6 | |
| 0.00 | 1.23 | 0.00 | 0.89 | 17.21 | 28.94 | -40.71 | 58.89 | 0.7300 | 184.0 | 62.9 | |
| 0.00 | 1.49 | 0.00 | 1.06 | 15.83 | 29.17 | -40.48 | 60.46 | 0.7202 | -593.0 | -510.8 | |
| 0.00 | 2.90 | 0.00 | 2.14 | 18.16 | 27.96 | -41.69 | 58.31 | 0.7450 | 687.0 | 485.1 | |
| 0.00 | 2.11 | 0.00 | 1.56 | 18.00 | 28.01 | -41.64 | 58.48 | 0.7436 | 470.0 | 395.9 | |
| 0.00 | 0.88 | 0.00 | 0.63 | 15.70 | 28.37 | -41.27 | 61.08 | 0.7278 | 604.0 | 559.3 | |
| 0.00 | 1.32 | 0.00 | 0.96 | 15.97 | 27.76 | -41.89 | 61.09 | 0.7356 | 529.0 | 486.5 | |
| 0.79 | 15.10 | 0.60 | 11.37 | 17.87 | 26.72 | -42.93 | 59.36 | 0.7556 | 570.7 | 506.8 | |
| 9.13 | -13.00 | 6.88 | -13.00 | 17.56 | 26.55 | -43.09 | 59.83 | 0.7557 | 754.9 | 999999 | |
| 0.00 | 0.88 | 0.00 | 0.66 | 17.18 | 26.06 | -43.59 | 60.55 | 0.7587 | 552.0 | 452.8 | |
| 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. | |