SDO HMI 2014-03-29 19:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.79 | 26.89 | 0.43 | 15.04 | 3.90 | 138.75 | 25.67 | 291.70 | 0.4671 | 87.4 | 269.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.61 | 0.00 | 0.35 | 4.84 | 142.07 | 28.99 | 290.97 | 0.5193 | -799.0 | -667.1 | |
| 0.00 | 1.49 | 0.00 | 0.86 | 5.54 | 141.97 | 28.89 | 292.29 | 0.5218 | -687.0 | -508.2 | |
| 0.00 | 1.23 | 0.00 | 0.70 | 3.45 | 141.70 | 28.62 | 288.67 | 0.5068 | -821.0 | -582.9 | |
| 0.00 | 1.40 | 0.00 | 0.80 | 2.83 | 141.44 | 28.37 | 287.67 | 0.5000 | -679.0 | -595.9 | |
| 0.00 | 1.84 | 0.00 | 1.06 | 5.12 | 141.54 | 28.46 | 291.85 | 0.5134 | -939.0 | -701.7 | |
| 0.00 | 0.44 | 0.00 | 0.25 | 6.49 | 141.41 | 28.33 | 294.40 | 0.5198 | -485.0 | -476.2 | |
| 0.00 | 1.40 | 0.00 | 0.81 | 7.11 | 140.36 | 27.28 | 296.36 | 0.5096 | -640.0 | -572.2 | |
| 0.00 | 2.54 | 0.00 | 1.41 | 2.92 | 138.62 | 25.54 | 289.84 | 0.4597 | 879.0 | 731.8 | |
| 0.79 | 5.78 | 0.43 | 3.18 | 2.41 | 137.32 | 24.24 | 289.78 | 0.4378 | 866.6 | 715.1 | |
| 0.00 | 3.41 | 0.00 | 1.89 | 4.57 | 137.38 | 24.30 | 294.23 | 0.4518 | 898.0 | 670.9 | |
| 0.00 | 2.98 | 0.00 | 1.65 | 3.80 | 137.29 | 24.21 | 292.75 | 0.4456 | 686.0 | 584.9 | |
| 0.00 | 1.75 | 0.00 | 0.97 | 4.29 | 137.24 | 24.16 | 293.79 | 0.4479 | 921.0 | 804.0 | |
| 0.00 | 0.44 | 0.00 | 0.24 | 2.67 | 137.13 | 24.05 | 290.51 | 0.4365 | 838.0 | 774.4 | |
| 0.00 | 1.58 | 0.00 | 0.87 | 3.73 | 137.09 | 24.01 | 292.78 | 0.4423 | 850.0 | 717.9 | |
| 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. | |